Modules for Experiments in Stellar Astrophysics (MESA)

Abstract

Stellar physics and evolution calculations enable a broad range of research in astrophysics. Modules for Experiments in Stellar Astrophysics (MESA) is a suite of open source libraries for a wide range of applications in computational stellar astrophysics. A newly designed 1-D stellar evolution module, MESA star, combines many of the numerical and physics modules for simulations of a wide range of stellar evolution scenarios ranging from very-low mass to massive stars, including advanced evolutionary phases. MESA star solves the fully coupled structure and composition equations simultaneously. It uses adaptive mesh refinement and sophisticated timestep controls, and supports shared memory parallelism based on OpenMP. Independently usable modules provide equation of state, opacity, nuclear reaction rates, and atmosphere boundary conditions. Each module is constructed as a separate Fortran 95 library with its own public interface. Examples include comparisons to other codes and show evolutionary tracks of very low mass stars, brown dwarfs, and gas giant planets; the complete evolution of a 1 Msun star from the pre-main sequence to a cooling white dwarf; the Solar sound speed profile; the evolution of intermediate mass stars through the thermal pulses on the He-shell burning AGB phase; the interior structure of slowly pulsating B Stars and Beta Cepheids; evolutionary tracks of massive stars from the pre-main sequence to the onset of core collapse; stars undergoing Roche lobe overflow; and accretion onto a neutron star. Instructions for downloading and installing MESA can be found on the project web site (http://mesa.sourceforge.net/).

110 pages, 39 figures; submitted to ApJS; visit the MESA website at http://mesa.sourceforge.net

References in corpus (64)

• Mass-loss predictions for O and B stars as a function of metallicity
• Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945
• A large stellar evolution database for population synthesis studies. I. Scaled solar models and isochrones
• A Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs
• Low Temperature Opacities
• The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$
• The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
• Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure
• Nucleosynthesis in Massive Stars With Improved Nuclear and Stellar Physics
• Astrophysical Reaction Rates From Statistical Model Calculations
• Galactic Chemical Evolution: Hydrogen Through Zinc
• The Theory of Brown Dwarfs and Extrasolar Giant Planets
• Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment
• Element Diffusion in the Solar Interior
• Approximate input physics for stellar modelling
• Theory of Low-Mass Stars and Substellar Objects
• Updated Electron-Conduction Opacities: The Impact on Low-Mass Stellar Models
• Kepler Asteroseismology Program: Introduction and First Results
• The ACS Survey of Galactic Globular Clusters. IX. Horizontal Branch Morphology and the Second Parameter Phenomenon
• The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• Helioseismology and Solar Abundances
• How Uncertain Are Solar Neutrino Predictions?
• Models for Type I X-Ray Bursts with Improved Nuclear Physics
• New Solar Composition: The Problem With Solar Models Revisited
• Helioseismological Implications of Recent Solar Abundance Determinations
• The ACS Survey of Galactic Globular Clusters. II. Stellar Evolution Tracks, Isochrones, Luminosity Functions, and Synthetic Horizontal-Branch Models
• ASTEC -- the Aarhus STellar Evolution Code
• Stellar evolution with rotation XII: Pre-supernova models
• SDSS unveils a population of intrinsically faint cataclysmic variables at the minimum orbital period
• S-factor of 14N(p,gamma)15O at astrophysical energies
• Thermodynamic functions of dense plasmas: analytic approximations for astrophysical applications
• CLES, Code Liegeois d'Evolution Stellaire
• The evolution of runaway stellar collision products
• YREC: The Yale Rotating Stellar Evolution Code
• Gallium Solar Neutrino Experiments: Absorption Cross sections, Neutrino spectra, and Predicted Event Rates
• On Validating an Astrophysical Simulation Code
• s-Process Nucleosynthesis in AGB Stars: A Test for Stellar Evolution
• CESAM: a free code for stellar evolution calculations
• Brown Dwarfs and the Cataclysmic Variable Period Minimum
• Massive Stars in the Range $13-25{\mathrm{M}}_{\odot }$: Evolution and Nucleosynthesis. II. the Solar Metallicity Models
• Asteroseismology of the Beta Cephei star Nu Eridani: Interpretation and applications of the oscillation spectrum
• Spectral models for solar-scaled and alpha-enhanced stellar populations
• Unstable Helium Shell Burning on Accreting White Dwarfs
• Exposing the Nuclear Burning Ashes of Radius Expansion Type I X-ray Bursts
• Lithium Depletion in Fully Convective Pre-Main Sequence Stars
• Models of Type I X-Ray Bursts in 4U 1820-30
• Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning
• Dust driven mass loss from carbon stars as a function of stellar parameters - I. A grid of Solar-metallicity wind models
• Deuterium-burning in substellar objects
• Dredge-up and envelope burning in intermediate mass giants of very low metallicity
• CoRoT's view of newly discovered B-star pulsators: results for 358 candidate B pulsators from the initial run's exoplanet field data
• The luminosity constraint on solar neutrino fluxes
• Low temperature Rosseland opacities with varied abundances of carbon and nitrogen
• Observational Tests and Predictive Stellar Evolution II: Non-standard Models
• The core helium flash revisited: II. Two and three-dimensional hydrodynamic simulations
• It's EZ to Evolve ZAMS Stars: A Program Derived from Eggleton's Stellar Evolution Code
• The C-flash and the ignition conditions of type Ia supernovae
• Low Mach Number Modeling of Type Ia Supernovae. IV. White Dwarf Convection
• Nuclear Reaction Rates and Carbon Star Formation
• Theoretical Uncertainties in Red Giant Branch Evolution: The Red Giant Branch Bump
• Models of Ultraluminous X-Ray Sources with Intermediate-Mass Black Holes
• On constructing horizontal branch models
• The CoRoT Evolution and Seismic Tools Activity: Goals and Tasks

Cited by in corpus (2864)

• A Massive Pulsar in a Compact Relativistic Binary
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
• Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
• Beyond the Cosmological Standard Model
• Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
• Modeling the Panchromatic Spectral Energy Distributions of Galaxies
• Kepler planets: a tale of evaporation
• The evaporation valley in the Kepler planets
• Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
• PARSEC evolutionary tracks of massive stars up to $350M_{\odot }$ at metallicities 0.0001$\le Z\le$0.04
• A new route towards merging massive black holes
• Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
• GYRE: An open-source stellar oscillation code based on a new Magnus Multiple Shooting Scheme
• The Evolution of Compact Binary Star Systems
• The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU
• Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
• Nominal values for selected solar and planetary quantities: IAU 2015 Resolution B3
• Nebular Continuum and Line Emission in Stellar Population Synthesis Models
• Hot subluminous stars
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• Wave-Driven Mass Loss in the Last Year of Stellar Evolution: Setting the Stage for the Most Luminous Core-Collapse Supernovae
• Slowing the Spins of Stellar Cores
• The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes
• On the age of the $\beta$ Pictoris moving group
• Probing the interior physics of stars through asteroseismology
• On the Spectral Evolution of Hot White Dwarf Stars. I. A Detailed Model-Atmosphere Analysis of Hot White Dwarfs from SDSS DR12
• The White Dwarf Initial-Final Mass Relation for Progenitor Stars From 0.85 to 7.5 M${}_{\odot }$
• Stellar cooling bounds on new light particles: plasma mixing effects
• Most Black Holes are Born Very Slowly Rotating
• One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
• Standing on the shoulders of Dwarfs: the Kepler asteroseismic LEGACY sample II - radii, masses, and ages
• A Compact Degenerate Primary-Star Progenitor of SN 2011fe
• COSMIC Variance in Binary Population Synthesis
• Super-Massive Stars as a Source of Abundance Anomalies of Proton-Capture Elements in Globular Clusters
• The Compactness of Presupernova Stellar Cores
• Angular momentum transport within evolved low-mass stars
• Cygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds
• Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes
• Discovery of a Candidate Black Hole - Giant Star Binary System in the Galactic Field
• Merging black hole binaries with the SEVN code
• How mergers magnetise massive stars
• Interrelated Main-Sequence Mass-Luminosity, Mass-Radius and Mass-Effective Temperature Relations
• Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk
• The 12C(a,g)16O reaction and its implications for stellar helium burning
• Asteroseismic classification of stellar populations among 13000 red giants observed by Kepler
• The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO
• Sub-Chandrasekhar-mass white dwarf detonations revisited
• Stellar structure models in modified theories of gravity: lessons and challenges
• High Resolution Study of Presupernova Compactness
• Three Hypervelocity White Dwarfs in Gaia DR2: Evidence for Dynamically Driven Double-Degenerate Double-Detonation Type Ia Supernovae
• Weighing Black Holes using Tidal Disruption Events
• An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D-HST Survey
• Photoevaporation and High-Eccentricity Migration Created the Sub-Jovian Desert
• The spin of the second-born black hole in coalescing binary black holes
• A new correction of stellar oscillation frequencies for near-surface effects
• Atmospheres of low-mass planets: the "boil-off"
• Evolutionary Analysis of Gaseous Sub-Neptune-Mass Planets with MESA
• NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Novae Supersoft Source
• The Long-Term Evolution of Double White Dwarf Mergers
• Pre-Supernova Outbursts via Wave Heating in Massive Stars I: Red Supergiants
• The Astrophysical Multipurpose Software Environment
• Super-luminous supernovae: 56Ni power versus magnetar radiation
• Constraints from gravitational wave detections of binary black hole mergers on the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ rate
• Setting the Stage for Circumstellar Interaction in Core-Collapse Supernovae II: Wave-Driven Mass Loss in Supernova Progenitors
• Concurrent formation of supermassive stars and globular clusters: implications for early self-enrichment
• An ancient extrasolar system with five sub-Earth-size planets
• Type II-Plateau supernova radiation: dependencies on progenitor and explosion properties
• The interior rotation of a sample of gamma Doradus stars from ensemble modelling of their gravity mode period spacings
• Stellar population synthesis based modelling of the Milky Way using asteroseismology of 13000 Kepler red giants
• Angular momentum transport by heat-driven g-modes in slowly pulsating B stars
• A Guide to Realistic Uncertainties on Fundamental Properties of Solar-Type Exoplanet Host Stars
• Short Gamma-Ray Bursts from the Merger of Two Black Holes
• Pulsational pair-instability supernovae in very close binaries
• A Sun-like star orbiting a black hole
• The Age and The Mass of The αHerculis Triple-Star System From A MESA Grid of rotating stars with 1.3 <= M/Msun <= 8.0
• Advanced burning stages and fate of 8-10 Mo stars
• Spectral models for binary products: Unifying Subdwarfs and Wolf-Rayet stars as a sequence of stripped-envelope stars
• A wide star-black-hole binary system from radial-velocity measurements
• Hydrodynamics of core-collapse supernovae and their progenitors
• Pulsating white dwarfs: new insights
• PTF12os and iPTF13bvn. Two stripped-envelope supernovae from low-mass progenitors in NGC 5806
• Tight asteroseismic constraints on core overshooting and diffusive mixing in the slowly rotating pulsating B8.3V star KIC 10526294
• Age dissection of the Milky Way discs: red giants in the Kepler field
• Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
• Astrophysical Tests of Modified Gravity: Constraints from Distance Indicators in the Nearby Universe
• Models of low-mass helium white dwarfs including gravitational settling, thermal and chemical diffusion, and rotational mixing
• PARSEC V2.0: Stellar tracks and isochrones of low and intermediate mass stars with rotation
• The Gaia-Kepler Stellar Properties Catalog. II. Planet Radius Demographics as a Function of Stellar Mass and Age
• A new mass-loss rate prescription for red supergiants
• Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
• Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. II. age dependencies and new insights
• The California-Kepler Survey. II. Precise Physical Properties of 2025 Kepler Planets and Their Host Stars
• Effects of Rotation on the Minimum Mass of Primordial Progenitors of Pair Instability Supernovae
• Stability of mass transfer from massive giants: double black-hole binary formation and ultra-luminous X-ray sources
• Measuring the Progenitor Masses and Dense Circumstellar Material of Type II Supernovae
• Improvements to stellar structure models, based on a grid of 3D convection simulations. II. Calibrating the mixing-length formulation
• NuGrid Stellar Data Set. II. Stellar Yields from H to Bi for Stellar Models with Mzams = 1 to 25Msun and Z = 0.0001 to 0.02
• New Insights into Classical Novae
• From the bulge to the outer disc: StarHorse stellar parameters, distances, and extinctions for stars in APOGEE DR16 and other spectroscopic surveys
• The role of mass transfer and common envelope evolution in the formation of merging binary black holes
• Type Ib and IIb supernova progenitors in interacting binary systems
• Seismic evidence for a weak radial differential rotation in intermediate-mass core helium burning stars
• Giant star seismology
• How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting
• Formation of black widows and redbacks -- two distinct populations of eclipsing binary millisecond pulsars
• A Multi-Mass Velocity Dispersion Model of 47 Tucanae Indicates No Evidence for an Intermediate Mass Black Hole
• Confirmation of the $Gaia$ DR2 parallax zero-point offset using asteroseismology and spectroscopy in the $Kepler$ field
• Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
• {\em Gaia}-derived luminosities of {\em Kepler} A/F stars and the pulsator fraction across the δ Scuti instability strip
• Sub-Inertial Gravity Modes in the B8V Star KIC 7760680 Reveal Moderate Core Overshooting and Low Vertical Diffusive Mixing
• Core rotation braking on the red giant branch for various mass ranges
• The influence of atomic diffusion on stellar ages and chemical tagging
• The delay of shock breakout due to circumstellar material seen in most Type II Supernovae
• Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry
• The impact of pair-instability mass loss on the binary black hole mass distribution
• SkyNet: A modular nuclear reaction network library
• Luminous Blue Variables and superluminous supernovae from binary mergers
• Constraining the initial entropy of directly-detected exoplanets
• A Grid of 3D Stellar Atmosphere Models of Solar Metallicity: I. General Properties, Granulation and Atmospheric Expansion
• Local Radiation Hydrodynamic Simulations of Massive Star Envelopes at the Iron Opacity Peak
• Different to the core: the pre-supernova structures of massive single and binary-stripped stars
• On the Orbits of Low-mass Companions to White Dwarfs and the Fates of the Known Exoplanets
• Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and ${}^{12}$C($\alpha$, $\gamma$)${}^{16}$O rate on the pair-instability black hole mass gap
• It has to be cool: on supergiant progenitors of binary black hole mergers from common-envelope evolution
• Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems
• The impact of mass-transfer physics on the observable properties of field binary black hole populations
• The Tidal Disruption of Giant Stars and Their Contribution to the Flaring Supermassive Black Hole Population
• Ionizing spectra of stars that lose their envelope through interaction with a binary companion: role of metallicity
• The expansion of stripped-envelope stars: consequences for supernovae and gravitational-wave progenitors
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations
• Age Determinations of the Hyades, Praesepe, and Pleiades via MESA Models with Rotation
• Overview of the DESI Milky Way Survey
• The Three Dimensional Evolution to Core Collapse of a Massive Star
• Pre-supernova evolution, compact object masses and explosion properties of stripped binary stars
• The Initiation and Propagation of Helium Detonations in White Dwarf Envelopes
• Stellar Models with Enhanced Abundances of C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti, in Turn, at Constant Helium and Iron Abundances
• The Thermonuclear Runaway and the Classical Nova Outburst
• Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
• The Origin of Black Hole Spin in Galactic Low-Mass X-ray Binaries
• A Systematic Survey of the Effects of Wind Mass Loss Algorithms on the Evolution of Single Massive Stars
• Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation
• Cool and Luminous Transients from Mass-Losing Binary Stars
• Stellar Multiplicity Meets Stellar Evolution And Metallicity: The APOGEE View
• Heartbeat Stars, Tidally Excited Oscillations, and Resonance Locking
• On the origin of W UMa type Contact binaries - a new method for computation of initial masses
• Dynamical Tides in Eccentric Binaries and Tidally-Excited Stellar Pulsations in KEPLER KOI-54
• Impact of type ia supernova ejecta on binary companions in the single-degenerate scenario
• Mass Transfer from Giant Donors
• An ultra-short period rocky super-Earth with a secondary eclipse and a Neptune-like companion around K2-141
• Planet Engulfment by ~1.5-3 Solar-Mass Red Giants
• Constructing A Flexible Likelihood Function For Spectroscopic Inference
• Pulsating red giant stars in eccentric binary systems discovered from Kepler space-based photometry
• The Revolution Revolution: magnetic morphology driven spin-down
• Stellar Evolution in AGN Disks
• Explosion of red-supergiant stars: influence of the atmospheric structure on shock breakout and the early-time supernova radiation
• A New Census of the 0.2 < z < 3.0 Universe, Part I: The Stellar Mass Function
• The asteroseismic potential of TESS: exoplanet-host stars
• The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age
• Stellar chromospheric activity of 1,674 FGK stars from the AMBRE-HARPS sample I. A catalogue of homogeneous chromospheric activity
• A comparison of evolutionary tracks for single Galactic massive stars
• A local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder
• Tidal dissipation in evolving low-mass and solar-type stars with predictions for planetary orbital decay
• LMXB and IMXB Evolution: I. The Binary Radio Pulsar PSR J1614-2230
• On the Origin of Black Hole Spin in High-mass X-Ray Binaries
• Radiative Properties of Pair-instability Supernova Explosions
• The Complete Evolution of a Neutron-Star Binary through a Common Envelope Phase Using 1D Hydrodynamic Simulations
• Characterising the observational properties of δ Sct stars in the era of space photometry from the Kepler mission
• Astrophysical Probes of the Vainshtein Mechanism: Stars and Galaxies
• Do electron-capture supernovae make neutron stars? First multidimensional hydrodynamic simulations of the oxygen deflagration
• On Variations Of Pre-Supernova Model Properties
• Constraining mixing in massive stars in the Small Magellanic Cloud
• Measuring the extent of convective cores in low-mass stars using Kepler data: towards a calibration of core overshooting
• On the sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars
• The Last Minutes of Oxygen Shell Burning in a Massive Star
• Angular Momentum Transport via Internal Gravity Waves in Evolving Stars
• Mass-accreting white dwarfs and type Ia supernovae
• Close Binary Companions to APOGEE DR16 Stars: 20,000 Binary-star Systems Across the Color-Magnitude Diagram
• Off the beaten path: Gaia reveals GD-1 stars outside of the main stream
• Skye: A Differentiable Equation of State
• Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
• KOI 1224, a Fourth Bloated Hot White Dwarf Companion Found With Kepler
• An Age Difference of 2 Gyr between a Metal-Rich and a Metal-Poor Globular Cluster
• Asymmetric Accretion Flows within a Common Envelope
• Nearly-uniform internal rotation of solar-like main-sequence stars revealed by space-based asteroseismology and spectroscopic measurements
• Characterization of exoplanets from their formation III: The statistics of planetary luminosities
• Tidal asteroseismology: Kepler's KOI-54
• Towards a better understanding of the evolution of Wolf-Rayet stars and Type Ib/Ic supernova progenitors
• The origin and evolution of magnetic white dwarfs in close binary stars
• GW150914: Spin based constraints on the merger time of the progenitor system
• Exploring the Potential Diversity of Early Type Ia Supernova Light Curves
• Bright, months-long stellar outbursts announce the explosion of interaction-powered supernovae
• Early formation and recent starburst activity in the nuclear disc of the Milky Way
• Tracing the formation of the Milky Way through ultra metal-poor stars
• Observable Signatures of Planet Accretion in Red Giant Stars I: Rapid Rotation and Light Element Replenishment
• Mass loss on the red giant branch: the value and metallicity dependence of Reimers' η in globular clusters
• Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution
• Deep Extragalactic VIsible Legacy Survey (DEVILS): SED Fitting in the D10-COSMOS Field and the Evolution of the Stellar Mass Function and SFR-$M_{\star }$ relation
• Super-Eddington Stellar Winds Driven by Near-Surface Energy Deposition
• A highly magnetised and rapidly rotating white dwarf as small as the Moon
• Constraining the Axion-Photon Coupling with Massive Stars
• Accretion in common envelope evolution
• Testing convective-core overshooting using period spacings of dipole modes in red giants
• Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge
• Analysis of broad-lined Type Ic supernovae from the (intermediate) Palomar Transient Factory
• Orbital properties of binary post-AGB stars
• Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions
• Every interacting double white dwarf binary may merge
• Solar structure and evolution
• Binary Population Synthesis
• Maximum Black Hole mass across Cosmic Time
• Very regular high-frequency pulsation modes in young intermediate-mass stars
• The Evolution and Fate of Super-Chandrasekhar Mass White Dwarf Merger Remnants
• Habitability of Terrestrial-Mass Planets in the HZ of M Dwarfs. I. H/He-Dominated Atmospheres
• An Overabundance of Black Hole X-Ray Binaries in the Galactic Center from Tidal Captures
• Common Envelope Wind Tunnel: Coefficients of Drag and Accretion in a Simplified Context for Studying Flows Around Objects Embedded Within Stellar Envelopes
• Oscillating red giants observed during Campaign 1 of the Kepler K2 mission: New prospects for galactic archaeology
• Beyond Mixing-length Theory: a step toward 321D
• Minimum Core Masses for Giant Planet Formation With Realistic Equations of State and Opacities
• Formation pathway of Population III coalescing binary black holes through stable mass transfer
• Pre-Supernova Outbursts via Wave Heating in Massive Stars II: Hydrogen-poor Stars
• Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN
• Towards a Realistic Explosion Landscape for Binary Population Synthesis
• Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy
• Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity
• Recombination energy in double white dwarf formation
• Determination of Three-dimensional Spin-orbit Angle with Joint Analysis of Asteroseismology, Transit Lightcurve, and the Rossiter-McLaughlin Effect: Cases of HAT-P-7 and Kepler-25
• Stellar-mass black holes in young massive and open stellar clusters IV: updated stellar-evolutionary and black hole spin models and comparisons with the LIGO-Virgo O1/O2 merger-event data
• Is HR 6819 a triple system containing a black hole? -- An alternative explanation
• Empirical Tidal Dissipation in Exoplanet Hosts From Tidal Spin-Up
• Magnetic massive stars as progenitors of "heavy" stellar-mass black holes
• Hydrogen-Poor Circumstellar Shells from Pulsational Pair-Instability Supernovae with Rapidly Rotating Progenitors
• Carbon-Oxygen Classical Novae are Galactic ${}^7$Li Producers as well as Potential Supernova Ia Progenitors
• Episodic accretion: the interplay of infall and disc instabilities
• Mass Ejection in Failed Supernovae: Variation with Stellar Progenitor
• Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates
• Modified Gravity Makes Galaxies Brighter
• Related progenitor models for long-duration gamma ray bursts and Type Ic superluminous supernovae
• Lessons from the Onset of a Common Envelope Episode: the Remarkable M31 2015 Luminous Red Nova Outburst
• N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift ?
• The dependence of convective core overshooting on stellar mass: Additional binary systems and improved calibration
• Black Hole Accretion Discs and Luminous Transients in Failed Supernovae from Non-Rotating Supergiants
• Conclusive evidence for a population of water-worlds around M-dwarfs remains elusive
• H ingestion into He-burning convection zones in super-AGB stellar models as a potential site for intermediate neutron-density nucleosynthesis
• Interacting Stellar EMRIs as Sources of Quasi-Periodic Eruptions in Galactic Nuclei
• The Formation of Jupiter's Diluted Core by a Giant Impact
• Three-Dimensional Simulations of Massive Stars: I. Wave Generation and Propagation
• The impact of stars stripped in binaries on the integrated spectra of stellar populations
• The Type IIb SN 2011dh - Two years of observations and modelling of the lightcurves
• Age Determination in Upper Scorpius with Eclipsing Binaries
• The Unusual Initial Mass Function of the Arches Cluster
• Hydrodynamic Simulations of the Interaction between Giant Stars and Planets
• Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection
• The Milky Way's nuclear star cluster: Old, metal-rich, and cuspy
• Forward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selection
• Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
• Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani
• Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004
• Asteroseismic modelling of the two F-type hybrid pulsators KIC10080943A and KIC10080943B
• The shape of convective core overshooting from gravity-mode period spacings
• The Low-Velocity, Rapidly Fading Type Ia Supernova 2002es
• Double Detonations with Thin, Modestly Enriched Helium Layers Can Make Normal Type Ia Supernovae
• The dependence of convective core overshooting on stellar mass: semi-empirical determination using the diffusive approach with two different element mixtures
• The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification
• On the Chemical Mixing Induced by Internal Gravity Waves (IGW)
• Is GW190521 the merger of black holes from the first stellar generations?
• Thermal Runaway During the Evolution of ONeMg Cores towards Accretion-Induced Collapse
• The mass discrepancy in intermediate- and high-mass eclipsing binaries: the need for higher convective core masses
• Isochrones for Old (> 5 Gyr) Stars and Stellar Populations. I. Models for $-2.4\le$ [Fe/H] $\le +0.6$, $0.25\le Y\le 0.33$, and $-0.4\le$ [$\alpha$\Fe] $\le +0.4$
• Turbulent Cold Flows Gave Birth to the First Quasars
• Pre-explosion spiral mass loss of a binary star merger
• On the Accretion-Fed Growth of Neutron Stars During Common Envelope
• Giant Impact: An Efficient Mechanism for the Devolatilization of Super-Earths
• Common envelope events with low-mass giants: understanding the transition to the slow spiral-in
• The Magnetic Furnace: Intense Core Dynamos in B-stars
• On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
• Measuring stellar and black hole masses of tidal disruption events
• Formation of Extremely Low-mass White Dwarfs in Double Degenerates
• Inferring Explosion Properties from Type II-Plateau Supernova Light Curves
• On the photometric detection of Internal Gravity Waves in upper main-sequence stars I. Methodology and application to CoRoT targets
• MESA Models of Classical Nova Outbursts: The Multicycle Evolution and Effects of Convective Boundary Mixing
• A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS
• X-ray Searches for Axions from Super Star Clusters
• "Retired" Planet Hosts: Not So Massive, Maybe Just Portly After Lunch
• The internal rotation profile of the B-type star KIC10526294 from frequency inversion of its dipole gravity modes and statistical model comparison
• Three Dimensional Radiation Hydrodynamic Simulations of Massive Star Envelopes
• Nuclear Physics of the Outer Layers of Accreting Neutron Stars
• Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in nuclear star clusters
• A Diversity of Wave-driven Pre-supernova Outbursts
• One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars
• Homogeneous Analysis of Hot Earths: Masses, Sizes, and Compositions
• The fate of fallback matter around newly born compact objects
• Uncertainties on near-core mixing in red-clump stars: effects on the period spacing and on the luminosity of the AGB bump
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Mixing by overshooting and rotation in intermediate mass stars
• Idealised hydrodynamic simulations of turbulent oxygen-burning shell convection in 4π geometry
• From Discovery to the First Month of the Type II Supernova 2023ixf: High and Variable Mass Loss in the Final Year before Explosion
• Non-radial oscillations in M-giant semi-regular variables: Stellar models and Kepler observations
• Stellar labels for hot stars from low-resolution spectra - I. the HotPayne method and results for 330,000 stars from LAMOST DR6
• Common envelope events with low-mass giants: understanding the energy budget
• Testing Screened Modified Gravity
• Circumstellar absorption in double detonation Type Ia supernovae
• A new class of pulsating white dwarf of extremely low mass: the fourth and fifth members
• Evolution of LMXBs under Different Magnetic Braking Prescriptions
• Predictions for the hydrogen-free ejecta of pulsational pair-instability supernovae
• The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae
• 3D NLTE spectral line formation of lithium in late-type stars
• Forward seismic modelling of the pulsating magnetic B-type star HD 43317
• Evolutionary Models for the Remnant of the Merger of Two Carbon-Oxygen Core White Dwarfs
• The C-flame Quenching by Convective Boundary Mixing in Super-AGB Stars and the Formation of Hybrid C/O/Ne White Dwarfs and SN Progenitors
• Immediate dense circumstellar environment of supernova progenitors caused by wind acceleration: its effect on supernova light curves
• Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
• Quasi-periodic eruptions from mildly eccentric unstable mass transfer in galactic nuclei
• Tidal Dissipation and Obliquity Evolution in Hot Jupiter Systems
• Massive donors in interacting binaries: effect of metallicity
• Detailed models of interacting short-period massive binary stars
• The Challenge of Forming a Fuzzy Core in Jupiter
• Detecting non-uniform period spacings in the Kepler photometry of gamma Doradus stars: methodology and case studies
• Fundamental Parameters of Main-Sequence Stars in an Instant with Machine Learning
• The i-process yields of rapidly-accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parameterizations from 3D hydrodynamics simulations
• Structural glitches near the cores of red giants revealed by oscillations in g-mode period spacings from stellar models
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• The dependence of convective core overshooting on stellar mass: reality check, and additional evidence
• Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars
• The Warm Neptune GJ 3470b has a Polar Orbit
• Asteroseismic signatures of evolving internal stellar magnetic fields
• Episodic mass ejections from common-envelope objects
• An algorithm for computing the 2D structure of fast rotating stars
• The Ecological Impact of High-performance Computing in Astrophysics
• Beyond the Standard Model Explanations of GW190521
• Tidal disruptions of main sequence stars -- III. Stellar mass dependence of the character of partial disruptions
• Three Ancient Halo Subgiants: Precise Parallaxes, Compositions, Ages, and Implications for Globular Clusters
• Iron Opacity Bump Changes the Stability and Structure of Accretion Disks in Active Galactic Nuclei
• An extended halo around an ancient dwarf galaxy
• 30 to 100-kG magnetic fields in the cores of red giant stars
• Detection of solar-like oscillations in relics of the Milky Way: asteroseismology of K giants in M4 using data from the NASA K2 mission
• Standing on the shoulders of giants: New mass and distance estimates for Betelgeuse through combined evolutionary, asteroseismic, and hydrodynamical simulations with MESA
• Spoon-Feeding Giant Stars to Supermassive Black Holes: Episodic Mass Transfer from Evolving Stars and Their Contribution to the Quiescent Activity of Galactic Nuclei
• The rise and fall of the Type Ib supernova iPTF13bvn - Not a massive Wolf-Rayet star
• Orbital evolution of mass-transferring eccentric binary systems. II. Secular Evolution
• TESS Hunt for Young and Maturing Exoplanets (THYME) VI: an 11 Myr giant planet transiting a very low-mass star in Lower Centaurus Crux
• Full-lifetime simulations of multiple unequal-mass planets across all phases of stellar evolution
• Type IIP supernova light curves affected by the acceleration of red supergiant winds
• Tidally-Induced Radius Inflation of Sub-Neptunes
• Helium abundance in a sample of cool stars: measurements from asteroseismology
• The Metastable Dynamo Model of Stellar Rotational Evolution
• Tidal Disruptions of Main Sequence Stars -- I. Observable Quantities and their Dependence on Stellar and Black Hole Mass
• Tidally-driven Roche-Lobe Overflow of Hot Jupiters with MESA
• How Many Components? Quantifying the Complexity of the Metallicity Distribution in the Milky Way Bulge with APOGEE
• Viscoelastic Tidal Dissipation in Giant Planets and Formation of Hot Jupiters Through High-Eccentricity Migration
• Gravitational Lensing of Gravitational Waves: Effect of Microlens Population in Lensing Galaxies
• Models of interacting supernovae and their spectral diversity
• Explaining the most energetic supernovae with an inefficient jet-feedback mechanism
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• Stellar mergers as the origin of the blue main-sequence band in young star clusters
• WASP-4b Arrived Early for the TESS Mission
• Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
• Diversity of common envelope jets supernovae and the fast transient AT2018cow
• A GRB and Broad-lined Type Ic Supernova from a Single Central Engine
• Evolution of Cataclysmic Variables and Related Binaries Containing a White-Dwarf
• Testing exoplanet evaporation with multi-transiting systems
• Envelope Convection, Surface Magnetism and Spots in A- and late B-type Stars
• Formation and evolution of hybrid He-CO white dwarfs and their properties
• On the photometric and spectroscopic diversity of Type II supernovae
• Formation channels of single and binary stellar-mass black holes
• Common envelopes in massive stars: Towards the role of radiation pressure and recombination energy in ejecting red supergiant envelopes
• KIC 10526294: a slowly rotating B star with rotationally split, quasi-equally spaced gravity modes
• Hunting Black Holes with Gaia
• Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS): Library of Fallback Rates
• Exact and approximate expressions of energy generation rates and their impact on the explosion properties of Pair Instability Supernovae
• Testing the radius scaling relation with $Gaia$ DR2 in the $Kepler$ field
• The Evolution and Properties of Rotating Massive Star Populations
• Efficient common-envelope ejection through dust-driven winds
• The Pristine Survey IV: Approaching the Galactic metallicity floor with the discovery of an ultra metal-poor star
• Ohmic Dissipation in the Interiors of Hot Jupiters
• Type Ia Single Degenerate Survivors Must Be Overluminous
• The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component
• Spin-orbit alignment of exoplanet systems: ensemble analysis using asteroseismology
• Long-term evolution of a magnetic massive merger product
• Toward a consistent use of overshooting parametrizations in 1D stellar evolution codes
• The Contour Method: a new approach to finding modes of non-adiabatic stellar pulsations
• Effects of close binary evolution on the main-sequence morphology of young star clusters
• Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi
• X-ray monitoring of classical novae in the central region of M31. III. Autumn and winter 2009/10, 2010/11 and 2011/12
• Asteroseismic estimate of helium abundance of a solar analog binary system
• The K2-HERMES Survey: Age and Metallicity of the Thick Disc
• The surface nitrogen abundance of a massive star in relation to its oscillations, rotation, and magnetic field
• KIC 3240411 - the hottest known SPB star with the asymptotic g-mode period spacing
• SPECULATOR: Emulating stellar population synthesis for fast and accurate galaxy spectra and photometry
• Non-Local Thermodynamic Equilibrium Radiative Transfer Simulations of Sub-Chandrasekhar-Mass White Dwarf Detonations
• Radii and Mass-loss Rates of Type IIb Supernova Progenitors
• Explaining iPTF14hls as a common envelope jets supernova
• The spins of compact objects born from helium stars in binary systems
• Period spacings of $\gamma$ Doradus pulsators in the \textit{Kepler} field: Rossby and gravity modes in 82 stars
• Improvements to Stellar Structure Models, Based on a Grid of 3D Convection Simulations. I. $T(\tau )$-Relations
• Chemical Abundances of Main-Sequence, Turn-off, Subgiant and red giant Stars from APOGEE spectra I: Signatures of Diffusion in the Open Cluster M67
• Evolution of Gas Giant Entropy During Formation by Runaway Accretion
• Chemically Homogeneous Evolution: A rapid population synthesis approach
• Evolutionary tracks for Betelgeuse
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum II. Test of a revised prescription for transport by the Tayler instability
• Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3
• On the Numerical Treatment and Dependence of Thermohaline Mixing in Red Giants
• Missing Red Supergiants and Carbon Burning
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• Post-merger evolution of carbon-oxygen + helium white dwarf binaries and the origin of R Coronae Borealis and extreme helium stars
• The Observational Signatures of Convectively Excited Internal Gravity Modes in Main Sequence Stars
• Metallicity-Dependent Signatures in the Kepler Planets
• Heating of the Intergalactic Medium by Hydrogen Reionization
• Recovering the star formation histories of recently-quenched galaxies: the impact of model and prior choices
• The Gaia-ESO Survey: open clusters in Gaia-DR1 - a way forward to stellar age calibration
• Predicting the Presence of Companions for Stripped-Envelope Supernovae: The Case of the Broad-Lined Type Ic SN 2002ap
• NS 1987A in SN 1987A
• SN 2009ib: A Type II-P Supernova with an Unusually Long Plateau
• Numerical Simulations of Convective 3-Dimensional Red Supergiant Envelopes
• Quasi-periodic Eruptions from Helium Envelope of Hydrogen-deficient Stars Stripped by Supermassive Black Holes
• A stripped-companion origin for Be stars: clues from the putative black holes HR 6819 and LB-1
• Confronting uncertainties in stellar physics: calibrating convective overshooting with eclipsing binaries
• Rotation of the convective core in $\gamma$ Dor stars measured by dips in period spacings of g modes coupled with inertial modes
• Hydrodynamic Simulations of the Interaction between an AGB Star and a Main Sequence Companion in Eccentric Orbits
• Chemical evolution library for galaxy formation simulation
• Gravity-mode period spacings and near-core rotation rates of 611 $\gamma$ Doradus stars with \textit{Kepler}
• Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
• Double-Peaked Balmer Emission Indicating Prompt Accretion Disk Formation in an X-Ray Faint Tidal Disruption Event
• On Carbon Burning in Super Asymptotic Giant Branch Stars
• Type II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling
• New Neutron-Capture Site in Massive Pop III and Pop II Stars as a Source for Heavy Elements in the Early Galaxy
• Massive star evolution : rotation, winds, and overshooting vectors in the Mass-Luminosity plane I. A calibrated grid of rotating single star models
• Coping with loss: Stability of mass transfer from post-main sequence donor stars
• Triggering jet-driven explosions of core-collapse supernovae by accretion from convective regions
• SN 2017ein and the Possible First Identification of a Type Ic Supernova Progenitor
• The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
• He-accreting carbon-oxygen white dwarfs and type Ia supernovae
• APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
• A strong shallow heat source in the accreting neutron star MAXI J0556-332
• On the Diversity of Fallback Rates from Tidal Disruption Events with Accurate Stellar Structure
• Orbital evolution of mass-transferring eccentric binary systems. I. Phase-dependent evolution
• The first ultracompact Roche lobe-filling hot subdwarf binary
• Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity
• The Dusty Progenitor Star of the Type II Supernova 2017eaw
• From Hot Jupiters to Super-Earths via Roche Lobe Overflow
• Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster
• Equation of state for magnetized Coulomb plasmas
• Dark Stars: A Review
• Modelling Kepler Red Giants in Eclipsing Binaries:Calibrating the Mixing Length Parameter with Asteroseismology
• Supernovae Ib and Ic from the explosion of helium stars
• Kepler-93b: A Terrestrial World Measured to within 120 km, and a Test Case for a New Spitzer Observing Mode
• Multi-Dimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin-Helium-Shell White Dwarfs
• Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system phi Persei
• New full evolutionary sequences of H and He atmosphere massive white dwarf stars using MESA
• The spin rate of pre-collapse stellar cores: wave-driven angular momentum transport in massive stars
• Ohmic Heating Suspends, not Reverses, the Cooling Contraction of Hot Jupiters
• The Ages of A-Stars I: Interferometric Observations and Age Estimates for Stars in the Ursa Major Moving Group
• The orbits of subdwarf-B + main-sequence binaries: III. The period - eccentricity distribution
• Tidal disruptions of main sequence stars -- II. Simulation methodology and stellar mass dependence of the character of full tidal disruptions
• Measuring mean densities of delta Scuti stars with asteroseismology. Theoretical properties of large separations using TOUCAN
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• Evolution Of Post-Impact Remnant Helium Stars In Type Ia Supernova Remnants Within The Single-Degenerate Scenario
• Convective turbulent viscosity acting on equilibrium tidal flows: new frequency scaling of the effective viscosity
• Stellar Oscillations in Modified Gravity
• Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
• The nature of the Li enrichment in the most Li-rich giant star
• Galactic Ultracompact X-ray Binaries: Disk Stability and Evolution
• Thermonuclear explosion of a massive hybrid HeCO white-dwarf triggered by a He-detonation on a companion
• Low Mass X-ray Binaries: The Effects of the Magnetic Braking Prescription
• Common-envelope evolution with an asymptotic giant branch star
• Constructing stable 3D hydrodynamical models of giant stars
• A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor
• Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution
• On the formation of PSR J1640+2224: a neutron star born massive?
• A Tendency Toward Alignment in Single-Star Warm Jupiter Systems
• Testing eccentricity pumping mechanisms to model eccentric long period sdB binaries with MESA
• NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z=0.01, Z=0.02 and Z=0.03
• Hubble Space Telescope survey of Magellanic Cloud star clusters. Photometry and astrometry of 113 clusters and early results
• The primordial and evolutionary abundance variations in globular-cluster stars: a problem with two unknowns
• Multidimensional Simulations of Rotating Pair Instability Supernovae
• Multi-Gigayear White Dwarf Cooling Delays from Clustering-Enhanced Gravitational Sedimentation
• Tidal Dissipation in WASP-12
• Was the nineteenth century giant eruption of Eta Carinae a merger event in a triple system?
• Progenitors of Type IIb Supernovae: I. Evolutionary Pathways and Rates
• A 20-Second Cadence View of Solar-Type Stars and Their Planets with TESS: Asteroseismology of Solar Analogs and a Re-characterization of pi Men c
• Multi-Dimensional Radiative Transfer Calculations of Double Detonations of Sub-Chandrasekhar-Mass White Dwarfs
• The limited role of recombination energy in common envelope removal
• Dispersal of protoplanetary disks by the combination of magnetically driven and photoevaporative winds
• Turbulence in Core-Collapse Supernovae
• Role of core-collapse supernovae in explaining Solar System abundances of p nuclides
• The Impact of Enhanced Iron Opacity on Massive Star Pulsations: Updated Instability Strips
• An Eccentric Massive Jupiter Orbiting a Sub-Giant on a 9.5 Day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images
• Accretion Disk Assembly During Common Envelope Evolution: Implications for Feedback and LIGO Binary Black Hole Formation
• Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
• MINESweeper: Spectrophotometric Modeling of Stars in the Gaia Era
• The Metallicity Dependence of the Minimum Mass for Core-Collapse Supernovae
• MESA and NuGrid simulations of classical novae: CO and ONe nova nucleosynthesis
• How stellar rotation shapes the colour magnitude diagram of the massive intermediate-age star cluster NGC 1846
• A Parameter-Space Study of Carbon-Oxygen White Dwarf Mergers
• Type II-Plateau supernovae as metallicity probes of the Universe
• Wait for it: Post-supernova winds driven by delayed radioactive decays
• The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: confirmation of HD 285507 b and refutation of AD Leo b
• 3D hydrodynamic simulations of C ingestion into a convective O shell
• An Accreting White Dwarf near the Chandrasekhar Limit in the Andromeda Galaxy
• An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary
• Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries and gravitational wave sources
• Binary Asteroseismic Modelling: isochrone-cloud methodology and application to Kepler gravity-mode pulsators
• Constraining stellar evolution theory with asteroseismology of $\gamma$ Doradus stars using deep learning
• Hybrid C-O-Ne white dwarfs as progenitors of type Ia supernovae: dependence on Urca process and mixing assumptions
• The surface abundances of Red Supergiants at core-collapse
• Probing the temperature gradient in the core boundary layer of stars with gravito-inertial modes: the case of KIC7760680
• The BAyesian STellar Algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology
• Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance
• Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7
• Evaporation of dark matter from celestial bodies
• The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
• Wave-driven stellar expansion and binary interaction in pre-supernova outbursts
• Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae
• The Tidal Disruption of Sun-like Stars by Massive Black Holes
• Unicorns and Giraffes in the binary zoo: stripped giants with subgiant companions
• Bayesian Estimation of Thermonuclear Reaction Rates
• Type II supernovae as probes of environment metallicity: observations of host HII regions
• Self-consistent predictions for LIER-like emission lines from post-AGB stars
• Analytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure
• Modeling protoplanetary disk SEDs with artificial neural networks: Revisiting the viscous disk model and updated disk masses
• Neutron star - white dwarf mergers: Early evolution, physical properties, and outcomes
• Orbital Decay of Short-Period Exoplanets via Tidal Resonance Locking
• X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
• Self-lensing Discovery of a $0.2M_{\odot }$ White Dwarf in an Unusually Wide Orbit Around a Sun-like Star
• Origin of W UMa-type contact binaries - age and orbital evolution
• Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
• Three-dimensional hydrodynamical simulations of mass transfer in binary systems by a free wind
• Non-detection of Helium in the Upper Atmospheres of Three Sub-Neptune Exoplanets
• Strong magnetic fields detected in the cores of 11 red giant stars using gravity-mode period spacings
• The Formation of a 70 Msun Black Hole at High Metallicity
• Planet populations inferred from debris discs: insights from 178 debris systems in the ISPY, LEECH and LIStEN planet-hunting surveys
• Structure and Evolution of Internally Heated Hot Jupiters
• Simulations of common envelope evolution in triple systems: Circumstellar case
• Stellar Structure and Tests of Modified Gravity
• Stellar and nebular diagnostics in the UV for star-forming galaxies
• Accretion onto Stars in the Disks of Active Galactic Nuclei
• The age-metallicity dependence for white dwarfs
• Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602
• Evolution of ONeMg Core in Super-AGB Stars towards Electron-Capture Supernovae: Effects of Updated Electron-Capture Rate
• Acoustic Signatures of the Helium Core Flash
• Triage of the Gaia DR3 astrometric orbits. I. A sample of binaries with probable compact companions
• Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow
• Influence of Nuclear Reaction Rate Uncertainties on Neutron Star Properties Extracted From X-ray Burst Model-Observation Comparisons
• An extremely energetic supernova from a very massive star in a dense medium
• An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561
• A precise asteroseismic age and metallicity for HD 139614: a pre-main-sequence star with a protoplanetary disc in Upper-Centaurus Lupus
• A Model for Fast Blue Optical Transient AT2018Cow: Circumstellar Interaction of a Pulsational Pair-instability Supernova
• The Effect of Supernova Convection On Neutron Star and Black Hole Masses
• The Planetary Accretion Shock. II. Grid of Post-Shock Entropies and Radiative Shock Efficiencies for Non-Equilibrium Radiation Transport
• iPTF15dtg: a double-peaked Type Ic Supernova from a massive progenitor
• Fingerprints of giant planets in the composition of solar twins
• Magnetic signatures on mixed-mode frequencies. I. An axisymmetric fossil field inside the core of red giants
• MESA meets MURaM: Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations
• The Close Binary Fraction as a Function of Stellar Parameters in APOGEE: A Strong Anti-Correlation With $\alpha$ Abundances
• Calibration of the Halpha Age-Activity relation for M dwarfs
• The Role of the Magnetorotational Instability in Massive Stars
• Evolved Massive Stars at Low-metallicity V. Mass-Loss Rate of Red Supergiant Stars in the Small Magellanic Cloud
• Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy
• Black hole-neutron star mergers are unlikely multi-messenger sources
• On the use of hydrogen recombination energy during common envelope events
• The effects of surface fossil magnetic fields on massive star evolution: II. Implementation of magnetic braking in MESA and implications for the evolution of surface rotation in OB stars
• The post-common envelope central stars of the planetary nebulae Henize 2-155 and Henize 2-161
• Properties and Evolution of the Redback Millisecond Pulsar Binary PSR J2129-0429
• Spitzer Follow-up of Extremely Cold Brown Dwarfs Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
• Understanding WASP-12b
• Re-evaluation of the ${}^{22}$Ne($\alpha ,\gamma$)${}^{26}$Mg and ${}^{22}$Ne($\alpha ,n$)${}^{25}$Mg reaction rates
• Formation of black holes in the pair-instability mass gap: evolution of a post-collision star
• On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars
• Revisiting nucleosynthesis in globular clusters: the case of NGC 2808 and the role of He and K
• Shock Breakout in 3-Dimensional Red Supergiant Envelopes
• Asteroseismic modelling of solar-type stars: internal systematics from input physics and surface correction methods
• Uncertainties in Galactic Chemical Evolution Models
• Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen Poor Low Mass White Dwarf
• A New Model of Roche-lobe Overflow for Short-Period Gaseous Planets and Binary Stars
• Asteroseismic modeling of 16 Cyg A & B using the complete Kepler data set
• Carbon Shell or Core Ignitions in White Dwarfs Accreting from Helium Stars
• Properties of Carbon-Oxygen White Dwarfs From Monte Carlo Stellar Models
• Tidal Inflation Reconciles Low-Density Sub-Saturns with Core Accretion
• Ultraviolet Detection of the Binary Companion to the Type IIb SN 2001ig
• Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity
• No cataclysmic variables missing: higher merger rate brings into agreement observed and predicted space densities
• The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
• The Effect of Tides on the Population of PN from Interacting Binaries
• Common envelope evolution of eccentric binaries
• Testing asteroseismology with Gaia DR2: Hierarchical models of the Red Clump
• No evidence for axions from Chandra observation of magnetic white dwarf
• Consistent Modeling of GS 1826-24 X-ray Bursts for Multiple Accretion Rates Demonstrates the Possibility to Constrain rp-process Reaction Rates
• Dynamical Tides in Compact White Dwarf Binaries: Helium Core White Dwarfs, Tidal Heating, and Observational Signatures
• The Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phase
• The difficulty of inferring progenitor masses from Type II-Plateau supernova light curves
• The very young resolved stellar populations around stripped-envelope supernovae
• Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars
• White dwarf binaries suggest a common envelope efficiency $\alpha \sim 1/3$
• The differential rotation of G dwarfs
• Rapid Rotation in the Kepler Field: Not a Single Star Phenomenon
• Long-rising Type II supernovae from PTF and CCCP
• PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
• Triple system HD 201433 with a SPB star component seen by BRITE-Constellation: Pulsation, differential rotation, and angular momentum transfer
• Dynamical Constraints on the Core Mass of Hot Jupiter HAT-P-13b
• Numerical Modeling of the Early Light Curves of Type IIP Supernovae
• POET: A Model for (P)lanetary (O)rbital (E)volution due to (T)ides on Evolving Stars
• The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at $z=5.4$ with JWST/NIRCam in GOODS-S
• Neutrinos from beta processes in a presupernova: probing the isotopic evolution of a massive star
• HARPS-N radial velocities confirm the low densities of the Kepler-9 planets
• Energy transport by convection in the common envelope evolution
• Modeling the early evolution of massive OB stars with an experimental wind routine
• Angular momentum transport in massive stars and natal neutron star rotation rates
• The single-sided pulsator CO~Camelopardalis
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
• Differential rotation and meridional flow on the lower zero age main sequence: Reynolds stress versus baroclinic flow
• The Most Massive Heartbeat: An In-depth Analysis of ι Orionis
• Evolution of Post-Impact Companion Stars in SN Ia Remnants within the Single-Degenerate Scenario
• Suppression of quadrupole and octupole modes in red giants observed by Kepler
• Radiative-transfer models for explosions from rotating and non-rotating single WC stars. Implications for SN1998bw and LGRB/SNe
• A two-stage formalism for common-envelope phases of massive stars
• Wolf-Rayet stars in the Small Magellanic Cloud as testbed for massive star evolution
• Low-frequency variability in massive stars: Core generation or surface phenomenon?
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• The Degree of Fine-Tuning in our Universe -- and Others
• Stellar Rotation in the K2 Sample: Evidence for Modified Spindown
• Hydrodynamical moving-mesh simulations of the tidal disruption of stars by supermassive black holes
• The Red-Giant Branch Bump Revisited: Constraints on Envelope Overshooting in a Wide Range of Masses and Metallicities
• Evolving LMXBs: CARB Magnetic Braking
• Low-mass White Dwarfs with Hydrogen Envelopes as a Missing Link in the Tidal Disruption Menu
• Internal rotation of 13 low-mass low-luminosity red giants in the Kepler field
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• Evolved Massive Stars at Low-metallicity I. A Source Catalog for the Small Magellanic Cloud
• A Compact Multi-Planet System With A Significantly Misaligned Ultra Short Period Planet
• Signatures of Mirror Stars
• Variability of Red Supergiants in M31 from the Palomar Transient Factory
• Transients from ONe White-Dwarf - Neutron-Star/Black-Hole Mergers
• Coupling thermal evolution of planets and hydrodynamic atmospheric escape in MESA
• TIC 168789840: A Sextuply-Eclipsing Sextuple Star System
• Tidal resonance locks in inspiraling white dwarf binaries
• The evolution of triples with a Roche-lobe filling outer star
• Electron Capture Supernovae From Close Binary Systems
• On the formation of eccentric millisecond pulsars with helium white-dwarf companions
• Surface-effect corrections for oscillation frequencies of evolved stars
• Pulsations of red supergiant pair-instability supernova progenitors leading to extreme mass loss
• KIC 4142768: An Evolved Gamma Doradus/Delta Scuti Hybrid Pulsating Eclipsing Binary with Tidally Excited Oscillations
• The effect of binding energy and resolution in simulations of the common envelope binary interaction
• Comprehensive study of ejecta-companion interaction for core-collapse supernovae in massive binaries
• Do R Coronae Borealis Stars Form from Double White Dwarf Mergers?
• Stellar ages, masses and radii from asteroseismic modeling are robust to systematic errors in spectroscopy
• Formation of Extremely Low-mass White Dwarfs Binaries
• The Role of Convection in Determining the Ejection Efficiency of Common Envelope Interactions
• How accurate are stellar ages based on stellar models ? I. The impact of stellar models uncertainties
• Asteroseismic inference of the near-core magnetic field strength in the main sequence B star HD 43317
• Spectroscopic Survey of γ Doradus Stars I. Comprehensive atmospheric parameters and abundance analysis of γ Doradus stars
• Collisional N-Body Dynamics Coupled to Self-Gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation
• Photoevaporative Dispersal of Protoplanetary Disks around Evolving Intermediate-mass Stars
• Resolving The Peak Of The Black Hole Mass Spectrum
• Searching For Rapid Orbital Decay of WASP-18b
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Combined Effects of Rotation and Age Spreads on Extended Main Sequence Turn Offs
• Dependence of Convective Boundary Mixing on Boundary Properties and Turbulence Strength
• Tidal Decay and Stable Roche-Lobe Overflow of Short-Period Gaseous Exoplanets
• Seismic measurement of the locations of the base of convection zone and helium ionization zone for stars in the {\it Kepler} seismic LEGACY sample
• Common Envelope Evolution on a Moving Mesh
• TOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star
• KIC 8164262: a Heartbeat Star Showing Tidally Induced Pulsations with Resonant Locking
• A nearby superluminous supernova with a long pre-maximum 'plateau' and strong CII features
• Tidal Downsizing model. I. Numerical methods: saving giant planets from tidal disruptions
• Simulating the formation of $\eta$ Carinae's surrounding nebula through unstable triple evolution and stellar merger-induced eruption
• Simulating a binary system that experiences the grazing envelope evolution
• On the Formation of Ultraluminous X-ray Sources with Neutron Star Accretors: the Case of M82 X-2
• The Dynamics of the Multi-planet System Orbiting Kepler-56
• A new class of Roche lobe-filling hot subdwarf binaries
• Discovery of post-mass-transfer helium-burning red giants using asteroseismology
• A helium-flash-induced mixing event can explain the lithium abundances of red clump stars
• Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
• A study of the low-luminosity Type II-Plateau supernova 2008bk
• Polluted White Dwarfs: Mixing Regions and Diffusion Timescales
• Constraints on the Initial-Final Mass Relation from Wide Double White Dwarfs
• The impact of recombination energy on simulations of the common envelope binary interaction
• Exploring the formation by core accretion and the luminosity evolution of directly imaged planets: The case of HIP 65426 b
• Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-Variable Horizontal-Branch Stars. I. M3, M15, and M92
• Screened fifth forces lower the TRGB-calibrated Hubble constant too
• Bipolar planetary nebulae from common envelope evolution of binary stars
• TOI-2109b: An Ultrahot Gas Giant on a 16 hr Orbit
• Turbulent Chemical Diffusion in Convectively Bounded Carbon Flames
• Variability of newly identified B-type stars observed by Kepler
• Missing in Action: New Physics and the Black Hole Mass Gap
• Prospects for asteroseismic inference on the envelope helium abundance in red giant stars
• WASP-4 is Accelerating Toward the Earth
• Constraints on explosive silicon burning in core-collapse supernovae from measured Ni/Fe ratios
• Discovery of Extended Main Sequence Turn-offs in Four Young Massive Clusters in the Magellanic Clouds
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• Statistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations
• Population synthesis of helium white dwarf--red giant star mergers and the formation of lithium-rich giants and carbon stars
• Study of Lithium Rich Giants with the GALAH Spectroscopic Survey
• Observed binary populations reflect the Galactic history. Explaining the orbital period-mass ratio relation in wide hot subdwarf binaries
• Light Curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers
• Are Super-Luminous supernovae and Long GRBs produced exclusively in young dense star clusters?
• KIC 9246715: The Double Red Giant Eclipsing Binary With Odd Oscillations
• The Uncertain Masses of Progenitors of Core Collapse Supernovae and Direct Collapse Black Holes
• Bow shock nebulae of hot massive stars in a magnetized medium
• Pre-collapse Properties of Superluminous Supernovae and Long Gamma-Ray Burst Progenitor Models
• Laterally Propagating Detonations in Thin Helium Layers on Accreting White Dwarfs
• Signatures of magnetic activity in the seismic data of solar-type stars observed by Kepler
• Orbital Evolution of Compact White Dwarf Binaries
• Magnetorotational core collapse of possible GRB progenitors. IV. A wider range of progenitors
• Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars
• How much hydrogen is in Type Ib and IIb supernova progenitors?
• Birth of the ELMs: a ZTF survey for evolved cataclysmic variables turning into extremely low-mass white dwarfs
• Rotation of Giant Stars
• An astrophysical interpretation of the remarkable g-mode frequency groups of the rapidly rotating $\gamma$ Dor star, KIC 5608334
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Planet-Mediated Precision-Reconstruction of the Evolution of the Cataclysmic Variable HU Aquarius
• Late time cooling of neutron star transients and the physics of the inner crust
• The evolution of CNO elements in galaxies
• The Value of Progenitor Radius Measurements for Explosion Modeling of Type II-Plateau Supernovae
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Discovery of Two New Thermally Bloated Low-Mass White Dwarfs Among the Kepler Binaries
• A new prescription for the mass-loss rates of WC and WO stars
• The Physical Parameters of the Retired A Star HD185351
• Neutrino Signal of Collapse-Induced Thermonuclear Supernovae: The Case for Prompt Black Hole Formation in SN1987A
• A new class of pulsating hot subdwarfs
• Asteroseismology of luminous red giants with Kepler I: Long Period Variables with radial and non-radial modes
• A He3 driven instability near the fully convective boundary
• PSR J1012+5307: a millisecond pulsar with an extremely low-mass white dwarf companion
• Benchmark ages for the Gaia benchmark stars
• Common envelope jets supernova (CEJSN) impostors resulting from a neutron star companion
• Subdwarf B stars from the common envelope ejection channel
• Rossby and Magnetic Prandtl Number Scaling of Stellar Dynamos
• Dynamical Tides in Highly Eccentric Binaries: Chaos, Dissipation and Quasi-Steady State
• Six New Compact Triply Eclipsing Triples Found With TESS
• A massive helium star with a sufficiently strong magnetic field to form a magnetar
• White-dwarf red-giant mergers, early-type R stars, J stars and lithium
• A Potential Progenitor for the Type Ic Supernova 2017ein
• Constraining the entropy of formation from young transiting planets
• Rotation in stellar interiors: General formulation and an asteroseismic-calibrated transport by the Tayler instability
• Hot subdwarfs formed from the merger of two He white dwarfs
• Uncertainties in s-process nucleosynthesis in low mass stars determined from Monte Carlo variations
• Convective core sizes in rotating massive stars: I. Constraints from solar metallicity OB field stars
• Ultra Long Gamma-Ray Bursts from the collapse of Blue Super Giant stars: an end-to-end simulation
• Extreme mass loss in low-mass type Ib/c supernova progenitors
• Binarity and beyond in A stars I. Survey description and first results of VLTI/GRAVITY observations of VAST targets with high Gaia-Hipparcos accelerations
• Bayesian Evolution Models for Jupiter with Helium Rain and Double-diffusive Convection
• Individual Alpha Elements, C, N, and Ba in Early Type Galaxies
• How to Make a Singleton sdB Star via Accelerated Stellar Evolution
• Very Massive Stars and Pair-Instability Supernovae: Mass-loss Framework for low Metallicity
• The Importance of Urca-process Cooling in Accreting ONe White Dwarfs
• Extended main-sequence turnoffs in the double cluster $h$ and $\chi$ Persei: The complex role of stellar rotation
• Planet Candidates from K2 Campaigns 5-8 and Follow-Up Optical Spectroscopy
• Kepler Eclipsing Binaries with $\delta$ Scuti/$\gamma$ Doradus Pulsating Components 1: KIC 9851944
• Excitation of gravity waves by fingering convection, and the formation of compositional staircases in stellar interiors
• The Milky Way tomography with APOGEE: intrinsic density distribution and structure of mono-abundance populations
• Stellar convective penetration: parameterized theory and dynamical simulations
• Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment
• Planetary Engulfment in the Hertzsprung--Russell Diagram
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• Convective Properties of Rotating Two-Dimensional Core-Collapse Supernova Progenitors
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Photometric properties of reionization-epoch galaxies in the Simba simulations
• How To Discover Mirror Stars
• Discrepancies in the ages of young star clusters; evidence for mergers?
• Population Synthesis of Black Hole X-Ray Binaries
• Angular momentum fluctuations in the convective helium shell of massive stars
• Asteroseismology of 36 Kepler subgiants -- II: Determining ages from detailed modelling
• Possible Origin of the G2 Cloud from the Tidal Disruption of a Known Giant Star by Sgr A*
• Measuring distances to low-luminosity galaxies using surface brightness fluctuations
• Constraining differential rotation of Sun-like stars from asteroseismic and starspot rotation periods
• Rejuvenated accretors have less bound envelopes: Impact of Roche lobe overflow on subsequent common envelope events
• MOST Observations of sigma Ori E: Challenging the Centrifugal Breakout Narrative
• Evolution of Wolf-Rayet stars as black hole progenitors
• Tidally Trapped Pulsations in Binary Stars
• Urca cooling pairs in the neutron star ocean and their effect on superbursts
• Alpha clustering and alpha-capture reaction rate from ab initio symmetry-adapted description of ${}^{20}$Ne
• On the survival of brown dwarfs and planets engulfed by their giant host star
• Feedback-Dominated Accretion Flows
• Radiative-transfer modeling of nebular-phase type II supernovae. Dependencies on progenitor and explosion properties
• Theoretical vs. observational uncertainties: composition of giant exoplanets
• Post main sequence evolution of icy minor planets: Implications for water retention and white dwarf pollution
• New and Known Moving Groups And Clusters Identified in a Gaia Co-Moving Catalog
• Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
• The TESS-Keck Survey I: A Warm Sub-Saturn-mass Planet and a Caution about Stray Light in TESS Cameras
• Ultra-compact X-ray binaries with He star companions
• KIC 8262223: A Post-Mass Transfer Eclipsing Binary Consisting of a Delta Scuti Pulsator and a Helium White Dwarf Precursor
• Searching for Li-rich giants in a sample of 12 open clusters: Li enhancement in two stars with substellar companions
• The COMBS Survey -- II. Distinguishing the Metal-Poor Bulge from the Halo Interlopers
• Progenitors of low-luminosity Type II-Plateau supernovae
• The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
• The Nearby Type Ibn Supernova 2015G: Signatures of Asymmetry and Progenitor Constraints
• Asteroseismology of red giants: from analysing light curves to estimating ages
• HATS-74Ab, HATS-75b, HATS-76b and HATS-77b: Four Transiting Giant Planets around K and M Dwarfs
• Asteroseismology of 3,642 Kepler Red Giants: Correcting the Scaling Relations based on Detailed Modeling
• Obtaining Precision Constraints on Modified Gravity with Helioseismology
• Comprehensive models of novae at metallicity $Z=0.02$ and $Z=10^{-4}$
• The Process of Stellar Tidal Disruption by Supermassive Black Holes. The first pericenter passage
• Giant planet formation models with a self-consistent treatment of the heavy elements
• Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
• Nucleosynthesis of binary-stripped stars
• Supermassive Dark Star candidates seen by JWST?
• The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
• Semi-analytic Expressions for the Isolation and Coupling of Mixed Modes
• Coupled Thermal and Compositional Evolution of Photo Evaporating Planet Envelopes
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• Stellar models with calibrated convection and temperature stratification from 3D hydrodynamics simulations
• Reproducing the observed abundances in RCB and HdC stars with post-double degenerate merger models - constraints on merger and post-merger simulations and physics processes
• Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352
• Faint rapid red transients from Neutron star -- CO white-dwarf mergers
• Stochastic Low Frequency Variability in 3-Dimensional Radiation Hydrodynamical Models of Massive Star Envelopes
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• The Effects of Curvature and Expansion on Helium Detonations on White Dwarf Surfaces
• The White Dwarf Binary Pathways Survey IV: Three close white dwarf binaries with G-type secondary stars
• Revisiting the explodability of single massive star progenitors of stripped-envelope supernovae
• Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia
• Three-Dimensional Hydrodynamic Simulations of Convective Nuclear Burning In Massive Stars Near Iron Core Collapse
• The asteroseismic surface effect from a grid of 3D convection simulations. I. Frequency shifts from convective expansion of stellar atmospheres
• Near-resonance in a system of sub-Neptunes from TESS
• Radiating the hydrogen recombination energy during common envelope evolution
• Can R CrB stars form from the merger of two helium white dwarfs?
• Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function
• Binary Interaction Dominates Mass Ejection in Classical Novae
• On the Origin of Sub-Subgiant Stars II: Binary Mass Transfer, Envelope Stripping, and Magnetic Activity
• Cold giant planets evaporated by hot white dwarfs
• Evolutionary models of red supergiants: Evidence for a metallicity-dependent mixing length and implications for Type IIP supernova progenitors
• A revisit of PSR J1909$-$3744 with 15-year high-precision timing
• Tidally Induced Pulsations in Kepler Eclipsing Binary KIC 3230227
• SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
• A new hydrodynamics code for Type Ia Supernovae
• Evolutionary models for R Coronae Borealis stars
• Updating the theoretical tidal evolution constants: Apsidal motion and the moment of inertia
• A physical model of mass ejection in failed supernovae
• TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full Frame Images
• HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2
• Increases to Inferred Rates of Planetesimal Accretion Due to Thermohaline Mixing in Metal Accreting White Dwarfs
• Gravity Modes Reveal the Internal Rotation of a Post-mass Transfer Gamma Doradus/Delta Scuti Hybrid Pulsator in Kepler Eclipsing Binary KIC 9592855
• Kepler Observations of the Asteroseismic Binary HD 176465
• Surviving companions of Type Ia supernovae: theory and observations
• Confronting uncertainties in stellar physics II. exploring differences in main-sequence stellar evolution tracks
• The Variability of the Star Formation Rate in Galaxies: I. Star Formation Histories Traced by EW(H$\alpha$) and EW(H${\delta }_A$)
• Accretion-Induced Collapse From Helium Star + White Dwarf Binaries
• Model-independent measurement of internal stellar structure in 16 Cygni A and B
• gyre_tides: Modeling binary tides within the gyre stellar oscillation code
• Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
• The effects of stellar rotation along the main sequence of the 100 Myr old massive cluster NGC 1850
• Analysis of apsidal motion in eclipsing binaries using TESS data II. A test of internal stellar structure}
• On the nature of rapidly fading Type II supernovae
• Tidally Induced Oscillations and Orbital Decay in Compact Triple-Star Systems
• The Most Metal-poor Stars in the Magellanic Clouds are $r$-process Enhanced
• Hydrodynamical simulations and similarity relations for eruptive mass loss from massive stars
• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
• Evolution models of helium white dwarf--main sequence star merger remnants
• A $75\%$ Occurrence Rate of Debris Discs around F stars in the $\beta$ Pic Moving Group
• Massive discs around low-mass stars
• Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition
• SN 2020jfo: A short plateau Type II supernova from a low mass progenitor
• Probing Final Stages of Stellar Evolution with X-Ray Observations of SN 2013ej
• Evolutionary modelling of subdwarf B stars using MESA with the predictive mixing and convective premixing schemes
• Modelling depletion by re-accretion of gas from a dusty disc in post-AGB stars
• Convective boundary mixing in main-sequence stars: theory and empirical constraints
• The Age of the Directly-Imaged Planet Host Star $\kappa$ Andromedae Determined From Interferometric Observations
• The Response of Giant Stars To Dynamical-Timescale Mass Loss
• Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Convective overshooting and penetration in a Boussinesq spherical shell
• TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars
• On the Formation of Galactic Black Hole Low-Mass X-ray Binaries
• Constraints on the distance moduli, helium and metal abundances, and ages of globular clusters from their RR Lyrae and non-variable horizontal-branch stars. II. Multiple stellar populations in 47Tuc, M3, and M13
• Star formation histories of the LEGUS dwarf galaxies (III): the non-bursty nature of 23 star forming dwarf galaxies
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• It takes a village to raise a tide: nonlinear multiple-mode coupling and mode identification in KOI-54
• Population synthesis of accreting white dwarfs: II. X-ray and UV emission
• On a new formulation for energy transfer between convection and fast tides with application to giant planets and solar type stars
• Emission from Pair-Instability Supernovae with Rotation
• A prescription for the asteroseismic surface correction
• The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
• Carbon-Oxygen Phase Separation in MESA White Dwarf Models
• Comparison of the optical light curves of hydrogen-rich and hydrogen-poor type II supernovae
• The response of a helium white dwarf to an exploding type Ia supernova
• Secular Dimming of KIC 8462852 Following its Consumption of a Planet
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• PTF1 J082340.04+081936.5: A hot subdwarf B star with a low mass white dwarf companion in an 87 minute orbit
• Dynamical Tides Reexpressed
• Presupernova neutrinos: realistic emissivities from stellar evolution
• Type Ib/Ic supernovae: effect of nickel mixing on the early-time color evolution and implications for the progenitors
• The Ages of Galactic Bulge Stars with Realistic Uncertainties
• Constraining Neutrino Cooling using the Hot White Dwarf Luminosity Function in the Globular Cluster 47 Tucanae
• Constraining massive star activities in the final years through properties of supernovae and their progenitors
• Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties
• Chronography of the Milky Way's Halo System with Field Blue Horizontal-Branch Stars
• PTF11mnb: the first analog of supernova 2005bf
• Ejection of globular cluster interstellar media through ionization by white dwarfs
• Screened Fifth Forces Mediated by Dark Matter-Baryon Interactions: Theory and Astrophysical Probes
• Polluting White Dwarfs with Perturbed Exo-Comets
• High-energy Cosmic Ray production in X-ray Binary Jets
• Low-temperature triple-alpha rate in a full three-body model
• Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries
• Tidal Circularization of Binaries by Resonance Locking I: The Importance of the Pre-Main-Sequence
• WDEC - A code for modeling white dwarf structure and pulsations
• Multiple stellar populations along the red Horizontal Branch and Red Clump of Globular Clusters
• Discovery of a double detonation thermonuclear supernova progenitor
• A simple and accurate prescription for the tidal disruption radius of a star and the peak accretion rate in tidal disruption events
• Evolution of intermediate-mass X-ray binaries driven by magnetic braking of Ap/Bp stars: I. ultracompact X-ray binaries
• KELT-25b and KELT-26b: A Hot Jupiter and a Substellar Companion Transiting Young A-stars Observed by TESS
• RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich
• Seismic signature of electron degeneracy in the core of red giants: hints for mass transfer between close red-giant companions
• High-Cadence, Early-Time Observations of Core-Collapse Supernovae From the TESS Prime Mission
• Insights into Tidal Disruption of Stars from PS1-10jh
• A Highly Eccentric 3.9-Millisecond Binary Pulsar in the Globular Cluster NGC 6652
• KIC 1718290: A Helium-rich V1093-Her-like Pulsator on the Blue Horizontal Branch
• Search for surviving companions in type Ia supernova remnants
• Synthetic Evolution Tracks of Giant Planets
• Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae
• Integrated Mass Loss of Evolved Stars in M4 using Asteroseismology
• Star formation in the first galaxies - III. Formation, evolution, and characteristics of the first stellar cluster
• Fundamental Properties of Co-Moving Stars observed by $Gaia$
• Properties of the Eclipsing Double-White Dwarf Binary NLTT 11748
• Properties of the post in-spiral common envelope ejecta II: dust formation
• A theoretical investigation of the Humphreys-Davidson limit at high and low metallicity
• Stellar wind models of subluminous hot stars
• Aluminium-26 from massive binary stars I: non-rotating models
• Gravito-inertial waves in a differentially rotating spherical shell
• Dynamical masses and mass-to-light ratios of resolved massive star clusters -- II. Results for 26 star clusters in the Magellanic Clouds
• Tidally Excited Oscillations in Heartbeat Binary Stars: Pulsation Phases and Mode Identification
• The Dusty and Extremely Red Progenitor of the Type II Supernova 2023ixf in Messier 101
• The role of radioactive nickel in shaping the plateau phase of Type II supernovae
• Numerical experiments to help understand cause and effect in massive star evolution
• Orbital Decay in Binaries Containing Post-Main Sequence Stars
• Wave-driven outbursts and variability of low-mass supernova progenitors
• Physical Properties of II Zw 40's Super Star Cluster and Nebula: New Insights and Puzzles from UV Spectroscopy
• From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers
• Type II supernovae from the Carnegie Supernova Project-I. I. Bolometric light curves of 74 SNe II using uBgVriYJH photometry
• The CubeSpec space mission. I. Asteroseismology of massive stars from time series optical spectroscopy: science requirements and target list prioritisation
• The statistical challenge of constraining the low-mass IMF in Local Group dwarf galaxies
• Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants
• Detecting axisymmetric magnetic fields using gravity modes in intermediate-mass stars
• Modeling Supermassive Primordial Stars with MESA
• The Cosmic Hunt for Members in the Outskirts of Ultra Faint Dwarf Galaxies: Ursa Major I, Coma Berenices, and Boötes I
• Binarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC
• Convective boundary mixing in a post-He core burning massive star model
• A sequence of Type Ib, IIb, II-L, and II-P supernovae from binary-star progenitors of varying initial separation
• Red Supergiants in M31 and M33 I. The Complete Sample
• The masses of retired A stars with asteroseismology: Kepler and K2 observations of exoplanet hosts
• Asymmetric Dark Matter May Alter the Evolution of Low-mass Stars and Brown Dwarfs
• A 3D radiation-hydrodynamic AGB binary model
• Photometric detection at $7.7\mu \mathrm{m}$ of a galaxy beyond redshift $14$ with JWST/MIRI
• Two-Dimensional Simulations of Internal Gravity Waves in The Radiation Zones of Intermediate-Mass Stars
• Phases of Mass Transfer from Hot Subdwarfs to White Dwarf Companions and Their Photometric Properties
• Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESA
• Asteroseismology of the Nearby SN-II Progenitor Rigel Part II. ε-Mechanism Triggering Gravity-Mode Pulsations?
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae
• Fundamental properties of Kepler and CoRoT targets: III. Tuning scaling relations using the first adiabatic exponent
• Analytic Models of Brown Dwarfs and The Substellar Mass Limit
• Observability of inflated companion stars after supernovae in massive binaries
• Relativistic Tidal Disruption and Nuclear Ignition of White Dwarf Stars by Intermediate Mass Black Holes
• Dynamical tides in exoplanetary systems containing Hot Jupiters: confronting theory and observations
• The Primordial Entropy of Jupiter
• Periodic accretion-powered flares from colliding EMRIs as TDE Imposters
• Common envelopes in massive stars II: The distinct roles of hydrogen and helium recombination
• The late type eclipsing binaries in the Large Magellanic Cloud: catalogue of fundamental physical parameters
• On The Development of Multidimensional Progenitor Models For Core-collapse Supernovae
• A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations
• Post-common-envelope binary stars, radiative levitation, and blue large-amplitude pulsators
• On the Origin of Solar Torsional Oscillations and Extended Solar Cycle
• Undetected Binary Stars Cause an Observed Mass Dependent Age Gradient in Upper Scorpius
• Accelerated Tidal Circularization Via Resonance Locking in KIC 8164262
• Mass discrepancy analysis for a select sample of Type II-Plateau supernovae
• Tidal Spin-up of Black Hole Progenitor Stars
• Explaining the differences in massive star models from various simulations
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• Radiation hydrodynamical simulations of eruptive mass Loss from progenitors of Type Ibn/IIn supernovae
• Testing White Dwarf Age Estimates using Wide Double White Dwarf Binaries from Gaia EDR3
• Surface effects on the red giant branch
• Carbon and Nitrogen Abundance Ratio In the Broad Line Region of Tidal Disruption Events
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• Numerical simulations of the random angular momentum in convection II: delayed explosions of red supergiants following "failed'' supernovae
• Mass loss of massive stars near the Eddington luminosity by core neutrino emission shortly before their explosion
• Pulsation in faint blue stars
• Shallower radius valley around low-mass hosts: Evidence for icy planets, collisions or high-energy radiation scatter
• A comparative analysis of the observed white dwarf cooling sequence from globular clusters
• Evolving R Coronae Borealis Stars with MESA
• Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au
• wdwarfdate: A Python Package to Derive Bayesian Ages of White Dwarfs
• The origins of Calcium-rich supernovae from disruptions of CO white-dwarfs by hybrid He-CO white-dwarfs
• MESA models with magnetic braking
• What are the spectroscopic binaries with high mass functions near the Gaia DR3 main sequence?
• A seismic scaling relation for stellar age
• High-precision asteroseismology in Slowly Pulsating B star: HD 50230
• Tidal disruptions of main sequence stars -- IV. Relativistic effects and dependence on black hole mass
• The cosmic carbon footprint of massive stars stripped in binary systems
• Optically Thin Core Accretion: How Planets Get Their Gas in Nearly Gas-Free Disks
• The spectral evolution of white dwarfs: where do we stand?
• Physics and evolution of the most massive stars in 30 Dor. Mass loss, envelope inflation, and a variable upper stellar mass limit
• Still Brighter than Pre-Explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart
• Wave-driven mass loss of stripped envelope massive stars: progenitor-dependence, mass ejection, and supernovae
• An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion
• Asteroseismic modeling of gravity modes in slowly rotating A/F stars with radiative levitation
• Hydrogen in hot subdwarfs formed by double helium white dwarf mergers
• Detailed chemical abundances of stars in the outskirts of the Tucana II ultra-faint dwarf galaxy
• Type Ia Supernova Explosions from Hybrid Carbon-Oxygen-Neon White Dwarf Progenitors
• Helium settling in F stars: constraining turbulent mixing using observed helium glitch signature
• Capture of stars into gaseous discs around massive black holes: Alignment, circularization and growth
• The initial physical conditions of Kepler-36 b & c
• The Betelgeuse Project: Constraints from Rotation
• Asteroseismic Fingerprints of Stellar Mergers
• Explaining Two Recent Intermediate Luminosity Optical Transients (ILOTs) by a Binary Interaction and Jets
• Enhancement of Lithium in Red Clump Stars by the Additional Energy Loss Induced by New Physics
• Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
• Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
• The Evolution of Rotation and Magnetic Activity in 94 Aqr Aa from Asteroseismology with TESS
• New mass-loss rates of B supergiants from global wind models
• Hot Start Giant Planets Form With Radiative Interiors
• The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
• Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
• Asteroseismology of the multiple stellar populations in the Globular Cluster M4
• Nonlinear dynamical tides in white dwarf binaries
• Radial Velocities of 41 Kepler Eclipsing Binaries
• Evidence for the preferential disruption of moderately massive stars by supermassive black holes
• Tidal Disruptions of Main Sequence Stars of Varying Mass and Age: Inferences from the Composition of the Fallback Material
• HIDES spectroscopy of bright detached eclipsing binaries from the $Kepler$ field - III. Spectral analysis, updated parameters, and new systems
• The Period-Luminosity Relations of Red Supergiants in M33 and M31
• On The Statistical Properties of the Lower Main Sequence
• A formation scenario for the triple pulsar PSR J0337+1715: breaking a binary system inside a common envelope
• KIC 7582608: A new Kepler roAp star with frequency variability
• A comparison of the dynamical and model-derived parameters of the pulsating eclipsing binary KIC9850387
• Mass ejection in failed supernovae: equation of state and neutrino loss dependence
• Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star
• The White Dwarf Binary Pathways Survey VI: two close post common envelope binaries with TESS light curves
• The White Dwarf Binary Pathways Survey -- VIII: a post common envelope binary with a massive white dwarf and an active G-type secondary star
• Internal rotation and inclinations of slowly pulsating B stars: Evidence of interior angular momentum transport
• Asteroseismic measurement of core and envelope rotation rates for 2006 red giant branch stars
• Wide post-common envelope binaries from Gaia: orbit validation and formation models
• The $\gamma$-process nucleosynthesis in core-collapse supernovae. I. A novel analysis of $\gamma$-process yields in massive stars
• Radiation shielding of protoplanetary discs in young star-forming regions
• Linking chromospheric activity and magnetic field properties for late-type dwarf stars
• Fast Blue Optical Transients due to Circumstellar Interaction and the Mysterious Supernova SN 2018gep
• PSR J1641+3627F: a low-mass He white dwarf orbiting a possible high-mass neutron star in the globular cluster M13
• Filling the Black Hole Mass Gap: Avoiding Pair Instability in Massive Stars through Addition of Non-Nuclear Energy
• Stellar Parameter Determination from Photometry using Invertible Neural Networks
• Re-inflation of warm and hot Jupiters
• Binary companions of evolved stars in APOGEE DR14: Orbital circularization
• Star Formation Histories of the LEGUS Dwarf Galaxies (I): recent History of NGC1705, NGC4449 and Holmberg II
• Supernovae from massive stars with extended tenuous envelopes
• Neutronization During Carbon Simmering In Type Ia Supernova Progenitors
• Is the Sulphur Anomaly in Planetary Nebulae Caused by the s-Process?
• The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution
• Tests of the asymptotic large frequency separation of acoustic oscillations in solar-type and red giant stars
• Stars stripped in binaries -- the living gravitational wave sources
• Stellar modelling of Spica, a high-mass spectroscopic binary with a beta Cep variable primary component
• Asteroseismic Signatures of Core Magnetism and Rotation in Hundreds of Low-Luminosity Red Giants
• SPYGLASS. III. The Fornax-Horologium Association and its Traceback History within the Austral Complex
• The double-peaked type Ic Supernova 2019cad: another SN 2005bf-like object
• Habitable Evaporated Cores and the Occurrence of Panspermia near the Galactic Center
• A relation between the radial velocity dispersion of young clusters and their age: Evidence for hardening as the formation scenario of massive close binaries
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. III. Using the rotation rates of intermediate-mass stars to test the Fuller-formalism
• On the frequency dependence of p-mode frequency shifts induced by magnetic activity in Kepler solar-like stars
• Tidally perturbed pulsations in the pre-main sequence $\delta$ Scuti binary RS Cha
• LAMOST Time-Domain Survey: First Results of four $K$2 plates
• Isochrone-cloud fitting of the extended Main-Sequence Turn-Off of young clusters
• An Atlas of Convection in Main-Sequence Stars
• On the Red Giant Branch: Ambiguity in the Surface Boundary Condition Leads to ~100 K Uncertainty in Model Effective Temperatures
• Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?
• Cosmic nucleosynthesis: a multi-messenger challenge
• Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collision
• Forward modeling of galaxy populations for cosmological redshift distribution inference
• Tess asteroseismology of the known planet host star ${\lambda }^2$ Fornacis
• The EBLM Project VI. The mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey
• Analysis of apsidal motion in eclipsing binaries using TESS data: I. A test of gravitational theories
• Supplying angular momentum to the jittering jets explosion mechanism using inner convection layers
• Formation of hot subdwarf B stars with neutron star components
• Eclipsing binaries in the open cluster Ruprecht 147. I: EPIC 219394517
• Is Betelgeuse the Outcome of a Past Merger?
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• Convection Destroys the Core/Mantle Structure in Hybrid C/O/Ne White Dwarfs
• Gravitational waves from in-spirals of compact objects in binary common-envelope evolution
• The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift
• The photometric variability of massive stars due to gravity waves excited by core convection
• Convection and Spin-Up During Common Envelope Evolution: The Formation of Short-Period Double White Dwarfs
• Five young $\delta$ Scuti stars in the Pleiades seen with Kepler/K2
• Upper Mass-Loss Limits and Clumping in the Intermediate and Outer Wind Regions of OB stars
• Tracking the evolution of lithium in giants using asteroseismology: Super-Li-rich stars are almost exclusively young red-clump stars
• Planet Engulfment Signatures in Twin Stars
• Disc-binary interactions in depleted post-AGB binaries
• A comparison of UV and optical metallicities in star-forming galaxies
• The OmegaWhite survey for short-period variable stars - V. Discovery of an ultracompact hot subdwarf binary with a compact companion in a 44 minute orbit
• Low-Temperature Gas Opacities with AESOPUS 2.0
• A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
• Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
• A Theoretical Study of Acoustic Glitches in Low-Mass Main-Sequence Stars
• Supernovae from direct collisions of white dwarfs and the role of helium shell ignition
• The first pre-supersoft X-ray binary
• The Araucaria Project. Accurate stellar parameters and distance to evolved eclipsing binary ASAS J180057-2333.8 in Sagittarius Arm
• A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
• Kepler Object of Interest Network II. Photodynamical modelling of Kepler-9 over 8 years of transit observations
• Main Sequence Evolution with Layered Semiconvection
• Constraining transport of angular momentum in stars: Combining asteroseismic observations of core helium burning stars and white dwarfs
• How does the mass and activity history of the host star affect the population of low-mass planets?
• Exploring the efficacy and limitations of shock-cooling models: new analysis of Type II supernovae observed by the Kepler mission
• Chemical Mixing Induced by Internal Gravity Waves in Intermediate Mass Stars
• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
• Progenitors of Type IIb Supernovae: II. Observable Properties
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• Formation of ultra-massive carbon-oxygen white dwarfs from the merger of carbon-oxygen and helium white dwarf pairs
• Failure of a neutrino-driven explosion after core-collapse may lead to a thermonuclear supernova
• First solar models with OPAS opacity tables
• Discovery of a disrupting open cluster far into the Milky Way halo: a recent star formation event in the leading arm of the Magellanic stream?
• Constraining axion-like particles using the white dwarf initial-final mass relation
• TOI-3235 b: a transiting giant planet around an M4 dwarf star
• Disk-fed giant planet formation
• Global 3D Radiation Hydrodynamic Simulations of Proto-Jupiter's Convective Envelope
• Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771
• Rapid evolution of the recurrence time in the repeating partial tidal disruption event eRASSt J045650.3-203750
• Improved Main Sequence Turnoff Ages of Young Open Clusters: Multicolor UBV Techniques & the Challenges of Rotation
• An ultra-short period rocky super-Earth orbiting the G2-star HD 80653
• Common Envelope Evolution on the Asymptotic Giant Branch: Unbinding within a Decade?
• Asteroseismology of 19 low-luminosity red giant stars from Kepler
• Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
• Predicted microlensing events from analysis of Gaia Data Release 2
• Properties of the radius valley around low mass stars: Predictions from the core-powered mass-loss mechanism
• Evolved Massive Stars at Low-metallicity III. A Source Catalog for the Large Magellanic Cloud
• Hydrodynamic Simulations of Pre-Supernova Outbursts in Red Supergiants: Asphericity and Mass Loss
• The progenitor of SN 2011ja: Clues from circumstellar interaction
• Long-Term Lithium Abundance Signatures following Planetary Engulfment
• The Binding Energy Parameter for Common Envelope Evolution
• Mitigating the mass dependence in the $\Delta \nu$ scaling relation of red-giant stars
• Heat transport and convective velocities in compositionally-driven convection in neutron star and white dwarf interiors
• Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all
• Convectively Driven Three Dimensional Turbulence in Massive Star Envelopes: I. A 1D Implementation of Diffusive Radiative Transport
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• Observations and three-dimensional ionization structure of the planetary nebula SuWt 2
• Atomic diffusion and turbulent mixing in solar-like stars: Impact on the fundamental properties of FG-type stars
• Modelling nova populations in galaxies
• The Tarantula Massive Binary Monitoring V. R 144: a wind-eclipsing binary with a total mass > 140 Msun
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Low-mass X-ray binaries from black-hole retaining globular clusters
• Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
• Supernova lightCURVE POPulation Synthesis II: Validation against supernovae with an observed progenitor
• Tidal disruption events from eccentric orbits and lessons learned from the noteworthy ASASSN-14ko
• Asteroseismology of the young open cluster NGC 2516 I: Photometric and spectroscopic observations
• New $\beta$ Cep pulsators discovered with K2 space photometry
• Masses of White Dwarf Binary Companions to Type Ia Supernovae Measured from Runaway Velocities
• The Continuing Story of SN IIb 2013df: New Optical and IR Observations and Analysis
• On the Red Supergiant Wind Kink. A Universal mass-loss concept for massive stars
• Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Weak shock propagation with accretion. I. Self-similar solutions and application to failed supernovae
• Neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy superluminous supernovae and Thorne-Żytkow objects
• Dark Matter Admixed Type Ia Supernovae
• Deep Learning Applied to the Asteroseismic Modeling of Stars with Coherent Oscillation Modes
• Shock breakouts from red supergiants: analytical and numerical predictions
• Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths
• The impact of realistic red supergiant mass-loss on stellar evolution
• Asteroseismic determination of fundamental parameters of sun-like stars using multi-layered neural networks
• Forming equatorial rings around dying stars
• Mass Transfer and Stellar Evolution of the White Dwarfs in AM CVn Binaries
• Validation of TESS exoplanet candidates orbiting solar analogues in the all-sky PLATO input catalogue
• A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
• A Bayesian Analysis of Physical Parameters for 783 Kepler (Near-)Contact Binaries: Extreme-Mass-Ratio Systems and a New Mass Ratio versus Period Lower Limit
• Predictions for gravity-mode periods and surface abundances in intermediate-mass dwarfs from shear mixing and radiative levitation
• Planets on the Edge
• Asteroseismic test of rotational mixing in low-mass white dwarfs
• On the pulsation modes of OGLE small amplitude red giant variables in the LMC
• Mass-Radius Relationships for Very Low Mass Gaseous Planets
• Post main sequence evolution of icy minor planets II: water retention and white dwarf pollution around massive progenitor stars
• Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A
• Asymmetric core collapse of rapidly rotating massive star
• Evolved Massive Stars at Low-metallicity II. Red Supergiant Stars in the Small Magellanic Cloud
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• Three-dimensional Hydrodynamics Simulations of Precollapse Shell Burning in the Si- and O-rich Layers
• Finding the First Cosmic Explosions. IV. 90 - 140 M${}_{\odot }$ Pair-Instability Supernovae
• Testing Gravity Theories Using Stars
• Stable mass transfer can explain massive binary black hole mergers with a high spin component
• Radial Velocity Discovery of an Eccentric Jovian World Orbiting at 18 au
• On the origin of nitrogen at low metallicity
• Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants
• Towards a new era in giant exoplanet characterisation
• Stellar Evolution Constraints on the Triple-Alpha Reaction Rate
• From the CMD of Omega Centauri and (super-)AGB stellar models to a Galactic plane passage gas purging chemical evolution scenario
• Sculpting the sub-Saturn Occurrence Rate via Atmospheric Mass Loss
• High Tide: A Systematic Search for Ellipsoidal Variables in ASAS-SN
• Helium Enhanced Planets Along the Upper Edge of the Radius Valley
• Another Shipment of Six Short-Period Giant Planets from TESS
• Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernova
• Period bouncers as detached magnetic cataclysmic variables
• The McDonald Accelerating Stars Survey (MASS): White Dwarf Companions Accelerating the Sun-like Stars 12 Psc and HD 159062
• Tango of celestial dancers: A sample of detached eclipsing binary systems containing g-mode pulsating components. A case study of KIC9850387
• Direct Detection of Atomic Dark Matter in White Dwarfs
• HE 0430-2457: a post merger extremely low-mass pre-white dwarf in a wide binary posing as an extreme horizontal branch star
• LAMOST J0140355+392651: An evolved cataclysmic variable donor transitioning to become an extremely low mass white dwarf
• The Role of the Magnetorotational Instability in the Sun
• Detecting Pair-Instability Supernovae at z<5 with the James Webb Space Telescope
• Asteroseismic g-mode period spacings in strongly magnetic rotating stars
• Stellar Pulsations in Beyond Horndeski Gravity Theories
• Evolution and final fate of massive post-common-envelope binaries
• Identification of the Optical Counterpart of Fermi Black Widow Millisecond Pulsar PSR J1544+4937
• A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae
• Electron-capture Rates in ${}^{20}$Ne for a Forbidden Transition to the Ground State of ${}^{20}$F Relevant to Final Evolution of High-density O-Ne-Mg Cores
• TESS Reveals HD 118203 b to be a Transiting Planet
• Deep HST Imaging in 47 Tucanae: A Global Dynamical Model
• Asymmetries of frequency splittings of dipolar mixed modes: a window on the topology of deep magnetic fields
• Convection Reconciles the Difference in Efficiencies Between Low-Mass and High-Mass Common Envelopes
• Novae heat their food: mass transfer by irradiation
• The long-term evolution and appearance of Type Iax postgenitor stars
• Nonlinear regimes in mean-field full-sphere dynamo
• Simulating highly-eccentric common envelope jets supernova (CEJSN) impostors
• Electron Captures on ${}^{14}\mathrm{N}$ as a Trigger for Helium Shell Detonations
• $\text{TESS}$ Giants Transiting Giants I: A Non-inflated Hot Jupiter Orbiting a Massive Subgiant
• Clumping and X-Rays in cooler B supergiant stars
• Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods
• Single-hemisphere dynamos in M-dwarf stars
• Black widow formation by pulsar irradiation and sustained magnetic braking
• Superadiabaticity and the metallicity independence of the Humphreys-Davidson limit
• A Dense Companion to the Short-Period Millisecond Pulsar Binary PSR J0636+5128
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• Dark Stars: Improved Models and First Pulsation Results
• Constraints on Bygone Nucleosynthesis of Accreting Neutron Stars
• Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence
• Imprint of planet formation in the deep interior of the Sun
• Horizontal shear instabilities in rotating stellar radiation zones: II. Effects of the full Coriolis acceleration
• On the impact of relativistic gravity on the rate of tidal disruption events
• Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer
• Close Encounters of Stars with Stellar-mass Black Hole Binaries
• The effects of diffusion in hot subdwarf progenitors from the common envelope channel
• Average opacity calculation for core-collapse supernovae
• Dynamical Mass of the Exoplanet Host Star HR 8799
• The Impact of White Dwarf Luminosity Profiles on Oscillation Frequencies
• Evidence of a signature of planet formation processes from solar neutrino fluxes
• Entropy Rain: Dilution and Compression of Thermals in Stratified Domains
• Effects of tidally enhanced stellar wind on the horizontal branch morphology of globular clusters
• The true stellar parameters of the Kepler target list
• Testing the cores of first ascent red-giant stars using the period spacing of g modes
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• Partial Tidal Disruption of Main-Sequence Stars by Intermediate-Mass Black Holes
• The first two-dimensional stellar structure and evolution models of rotating stars
• Accumulated Tidal Heating of Stars Over Multiple Pericenter Passages Near SgrA*
• Seismic modeling of a very young SPB star -- KIC8264293
• Short Term Variability of Evolved Massive Stars with TESS
• The blue straggler V106 in NGC6791: A prototype progenitor of old single giants masquerading as young
• The effects of near-core convective shells on the gravity modes of the subdwarf B pulsator KIC 10553698A
• SCExAO and GPI $YJH$ Band Photometry and Integral Field Spectroscopy of the Young Brown Dwarf Companion to HD 1160
• GRaM-X: A new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling With ALMA
• Modified Gravity and the Black Hole Mass Gap
• Common envelope binary interaction simulations between a thermally-pulsating AGB star and a low mass companion
• Velocity limits in the thermonuclear supernova ejection scenario for hypervelocity stars and the origin of US 708
• Effects of Irradiation on the Evolution of Ultra-compact X-ray Binaries
• Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115
• Convective Mixing in Gas Giant Planets with Primordial Composition Gradients
• Isochronal age-mass discrepancy of young stars: SCExAO/CHARIS integral field spectroscopy of the HIP 79124 triple system
• Searching for dark energy with the Sun
• The Loudest Stellar Heartbeat: Characterizing the most extreme amplitude heartbeat star system
• Planet-Induced Stellar Pulsations in HAT-P-2's Eccentric System
• Metal-Rich SX Phe stars in the Kepler Field
• Extreme isolation of WN3/O3 stars and implications for their evolutionary origin as the elusive stripped binaries
• Supernova explosions interacting with aspherical circumstellar material: implications for light curves, spectral line profiles, and polarization
• Warm millimetre dust in protoplanetary discs near massive stars
• Three long period transiting giant planets from TESS
• Magnetic braking with MESA evolutionary models in the single star and LMXB regimes
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• The magneto-rotational instability in massive stars
• Explodability criteria for the neutrino-driven supernova mechanism
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• Recovery from Giant Eruptions in Very Massive Stars
• Evaporation Barrier for Dark Matter in Celestial Bodies
• Gravity mode offset and properties of the evanescent zone in red-giant stars
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• WOCS 5379: Detailed Analysis of the Evolution of a Post-Mass-Transfer Blue Straggler
• SN 2022acko: the First Early Far-Ultraviolet Spectra of a Type IIP Supernova
• The IACOB project IX. Building a modern empirical database of Galactic O9-B9 supergiants: sample selection, description, and completeness
• 3D1D hydro-nucleosynthesis simulations. I. Advective-reactive post-processing method and its application to H ingestion into He-shell flash convection in rapidly accreting white dwarfs
• New asteroseismic scaling relations based on Hayashi track relation applied to red-giant branch stars in NGC 6791 and NGC 6819
• Two decades of optical timing of the shortest-period binary star system HM Cancri
• On the energy source of ultra-stripped supernovae
• Cycle period, differential rotation and meridional flow for early M dwarf stars
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• The Impact of Progenitor Mass Loss on the Dynamical and Spectral Evolution of Supernova Remnants
• The outcomes of carbon-oxygen white dwarfs accreting CO-rich material
• Hierarchically modelling Kepler dwarfs and subgiants to improve inference of stellar properties with asteroseismology
• On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram
• Spatio-kinematic modelling of Abell 65, a double-shelled planetary nebula with a binary central star
• WIYN Open Cluster Study. LXXXVII. HST Ultraviolet Detection of Hot White Dwarf Companions to Blue Lurkers in M67
• Magnetic field breakout from white dwarf crystallization dynamos
• Accounting for planet-shaped planetary nebulae
• Burst-induced coronal cooling in GS 1826-24 The clock wagging its tail
• X-Ray emission from SN 2004dj: A Tale of Two Shocks
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• X-Shooting ULLYSES: Massive Stars at low metallicity VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
• The HST large programme on $\omega$ Centauri -- V. Exploring the Ultracool Dwarf Population with Stellar Atmosphere and Evolutionary Modelling
• KIC 10736223: An Algol-type eclipsing binary just undergone the rapid mass-transfer stage
• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• KELT-24b: A 5M${}_{\mathrm{J}}$ Planet on a 5.6 day Well-Aligned Orbit around the Young V=8.3 F-star HD 93148
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• A Study of Nine Triply Eclipsing Triples
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters From Their RR Lyrae and Non-Variable Horizontal-Branch Stars. III. M55 and NGC 6362
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• Nature vs. Nurture: Distinguishing Effects from Stellar Processing and Chemical Evolution on Carbon and Nitrogen in Red Giant Stars
• Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds from ASAS-SN: Implications for Thorne-Żytkow Objects and Super-Asymptotic Giant Branch Stars
• A possible formation channel for blue hook stars in globular cluster
• GASTLI: An open-source coupled interior-atmosphere model to unveil gas giant composition
• A synthetic sample of short-cadence solar-like oscillators for TESS
• A red giant branch common envelope evolution scenario for the exoplanet WD 1856 b
• Isochrone fitting of Galactic globular clusters - I. NGC 5904
• Onset of Nonlinear Internal Gravity Waves in Intermediate-Mass Stars
• The Radius and Entropy of a Magnetized, Rotating Fully-convective Star: Analysis With Depth-dependent Mixing Length Theories
• Gaia-based Isochronal, Kinematic, and Spatial Analysis of the $\epsilon$ Cha Association
• A close-in giant planet escapes engulfment by its star
• A Model for Clumpy Self-Enrichment in Globular Clusters
• Modeling overcontact binaries, I. The effect of tidal deformation
• Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
• Monte-Carlo methods for NLTE spectral synthesis of supernovae
• Modelling the Milky Way. I -- Method and first results fitting the thick disk and halo with DES-Y3 data
• The ASAS-SN Catalog of Variable Stars VIII: "Dipper" Stars in the Lupus Star-Forming Region
• Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier?
• Population of post-nova supersoft X-ray sources
• Accreting CO material onto ONe white dwarfs towards accretion-induced collapse
• Dynamical Masses and Stellar Evolutionary Model Predictions of M-Stars
• Inverse Tides in Pulsating Binary Stars
• On the existence of brown dwarfs more massive than the hydrogen burning limit
• Surface correction of main sequence solar-like oscillators with the $Kepler$ LEGACY sample
• ASASSN-14dq: A fast-declining type II-P Supernova in a low-luminosity host galaxy
• An Analytical Density Profile of Dense Circumstellar Medium in Type II Supernovae
• Determining the seismic age of the young open cluster $\alpha$ Per using $\delta$ Scuti stars
• Spectroscopic study of two new super Li rich red clump K giants
• Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• Spin and Magnetism of White Dwarfs
• Masses, Oxygen and Carbon abundances in CHEPS dwarf stars
• Energy Budget and Core-Envelope Motion in Common Envelope Evolution
• Detecting deep axisymmetric toroidal magnetic fields in stars. The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field
• The Asteroseismic Imprints of Mass Transfer: A Case Study of a Binary Mass Gainer in the SPB Instability Strip
• The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
• The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints
• An accurate and efficient numerical calculation of detonation waves in multidimensional supernova simulations using a burning limiter and adaptive quasi-statistical equilibrium
• Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
• Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
• Benchmarking MESA isochrones against the Hyades single star sequence
• A Super-Eddington Wind Scenario for the Progenitors of Type Ia Supernovae
• A theory of mass transfer in binary stars
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• High-temperature ${}^{205}$Tl decay clarifies ${}^{205}$Pb dating in early Solar System
• 3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
• Asteroseismology of the Hyades with K2: first detection of main-sequence solar-like oscillations in an open cluster
• Contamination in TESS light curves: The case of the Fast Yellow Pulsating Supergiants
• The Blue Stragglers of the Old Open Cluster NGC 188
• beta Cas: the first delta Scuti star with a dynamo magnetic field
• The role of stellar expansion on the formation of gravitational wave sources
• Influence of a mass transfer stability criterion on double white dwarf populations
• Optically thin circumstellar medium in $\beta$ Lyr A system
• Modeling contact binaries, II. The effect of energy transfer
• SPYGLASS. II. The Multi-Generational and Multi-Origin Star Formation History of Cepheus Far North
• Precursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae
• What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST
• Modelling of Sigma Scorpii, a high-mass binary with a Beta Cep variable primary component
• Eclipsing Systems with Pulsating Components (Types β Cep, δ Sct, γ Dor or Red Giant) in the Era of High-Accuracy Space Data
• Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion
• Asteroseismic Inference of Subgiant Evolutionary Parameters with Deep Learning
• A Measurement of Diffusion in 47 Tucanae
• Orbital Motion of Young Binaries in Ophiuchus and Upper Centaurus-Lupus
• Type Ia supernovae from non-accreting progenitors
• A theoretical framework of BL Her stars. I. Effect of metallicity and convection parameters on period-luminosity and period-radius relations
• Observational Constraints on the Common Envelope Phase
• Tidal migration of hot Jupiters: introducing the impact of gravity wave dissipation
• Is Thermohaline Mixing the Full Story? Evidence for Separate Mixing Events near the Red Giant Branch Bump
• The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
• Residual Carbon in Oxygen-Neon White Dwarfs and its Implications for Accretion-Induced Collapse
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• Revising Properties of Planet-Host Binary Systems. III. There is No Observed Radius Gap For Kepler Planets in Binary Star Systems
• Searching for the Donor Stars of ULX Pulsars
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• Radiative Acceleration of Dense Circumstellar Material in Interacting Supernovae
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• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. I. Confirmation of an Eccentric, Cool Jupiter With an Interior Earth-sized Planet Orbiting Kepler-1514
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• Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars
• A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• Solar dynamo cycle variations with a rotational period
• Stochastic excitation of internal gravity waves in rotating late F-type stars: A 3D simulation approach
• DES16C3cje: A low-luminosity, long-lived supernova
• A Nitrogen-Enhanced Metal-Poor star discovered in the globular cluster ESO280-SC06
• Structural and Evolutionary Diagnostics from Asteroseismic Phase Functions
• The evolution of circumstellar discs in the Galactic Centre: an application to the G-clouds
• The Three-Dimensional Collapse of a Rapidly Rotating 16 $M_{\odot }$ Star
• A Transparent Window into Early-Type Stellar Variability
• Signatures of a surviving helium-star companion in Type Ia supernovae and constraints on the progenitor companion of SN 2011fe
• Sensitivity of Carbon and Oxygen Yields to the Triple-Alpha Resonance in Massive Stars
• The impact of the uncertainties in the 12C(α,γ)16O reaction rate on the evolution of low- to intermediate-mass stars
• A new C-D-like diagram for SPB stars: The variations of period spacing as a signature of evolutionary status
• Minimum Orbital Period of Pre-Cataclysmic Variables
• Cooling Models for the Most Massive White Dwarfs
• The first heavy-metal hot subdwarf composite binary SB 744
• A Study of Wolf-Rayet stars Formed via Chemically Homogeneous Evolution
• A Circumbinary Disk Model for the Rapid Orbital Shrinkage in Black Hole Low-Mass X-ray Binaries
• Orbital and physical parameters of eclipsing binaries from the ASAS catalogue -- XII. A sample of systems with $K2$ photometry
• Radio observations of massive stars in the Galactic centre: The Arches Cluster
• Pulsations of the High-Amplitude $\delta$ Scuti Star YZ Bootis
• Towards a fully consistent Milky Way disk model -- IV. The impact of Gaia DR2 and APOGEE
• Rotation and Magnetism of Massive Stellar Cores
• The formation of type Ia supernovae from carbon-oxygen-silicon white dwarfs
• The impact of composition choices on solar evolution: age, helio- and asteroseismology, and neutrinos
• Exploring the convective core of the hybrid $\delta$ Scuti-$\gamma$ Doradus star CoRoT 100866999 with asteroseismology
• Mirror principle and the red-giant bump: the battle of entropy in low-mass stars
• Three new barium dwarfs with WD companions: BD+68 1027, RE J0702+129 and BD+80 670
• Asteroseismology of the $\delta$ Scuti star HD 50844
• An evolutionary channel towards the accreting millisecond pulsar SAX J1808.4-3658
• Binary white dwarfs in the halo of the Milky Way
• Should I Stay or Should I Go: Stellar Wind Retention and Expulsion in Massive Star Clusters
• The Thermal Stability of Helium Burning on Accreting Neutron Stars
• Evolution and Nucleosynthesis of Very Massive Stars
• Blue Stragglers and Friends: Initial Evolutionary Pathways in Close Low-Mass Binaries: Literature Review
• An absolute mass, precise age, and hints of planetary winds for WASP-121 A and b from a JWST NIRSpec phase curve
• Tides in the high-eccentricity migration of hot Jupiters: Triggering diffusive growth by nonlinear mode interactions
• Unraveling the evolution of hot Jupiter systems under the effect of tidal and magnetic interactions and mass loss
• The effect of the adiabatic assumption on asteroseismic scaling relations for luminous red giants
• Off-axis synchrotron light curves from full-time-domain moving-mesh simulations of jets from massive stars
• Platform for Probing Radiation Transport Properties of Hydrogen at Conditions Found in the Deep Interiors of Red Dwarfs
• Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• A possible formation channel for blue hook stars in globular cluster - II. Effects of metallicity, mass ratio, tidal enhancement efficiency and helium abundance
• Rotational modulation in A and F stars: Magnetic stellar spots or convective core rotation?
• Effects of axions on Nucleosynthesis in massive stars
• The hydrogen clock to infer the upper stellar mass
• Formation of black hole X-ray binaries with non-degenerate donors in globular clusters
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey: III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-Transit Jupiter Orbiting TOI-2010
• Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars. Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models
• Three Dimensional Natures of Massive Star Envelopes
• General Relativistic Hydrodynamics on a Moving-mesh I: Static Spacetimes
• Multiple stellar populations at less evolved stages: detection of chemical variations among main-sequence dwarfs in NGC 1978
• The mass distribution of stars stripped in binaries: The effect of metallicity
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Impact of binary interaction on the evolution of blue supergiants
• Properties of the Hyades, the eclipsing binary HD27130, and the oscillating red giant $\epsilon$ Tau
• Nonkinematic solar dynamo models with double-cell meridional circulation
• {\it Gaia} DR2 giants in the Galactic dust -- I. Reddening across the whole dust layer and some properties of the giant clump
• The evolution of catastrophically evaporating rocky planets
• Modeling of multimode radially pulsating High-Amplitude Delta Scuti stars from the OGLE Galactic bulge sample
• SMA detection of an extreme millimeter flare from the young class III star HD 283572
• Cyberhubs: Virtual Research Environments for Astronomy
• Towards a more rigorous treatment of uncertainties on the velocity distribution of dark matter particles for capture in stars
• The bulk metallicity of giant planets around M stars
• A 5% measurement of the gravitational constant in the Large Magellanic Cloud
• Pulsation-driven mass loss from massive stars behind stellar mergers in metal-poor dense clusters
• Empirical instability strip for classical Cepheids: I. The LMC galaxy
• Pulse Profile Modeling of Thermonuclear Burst Oscillations I: The Effect of Neglecting Variability
• Multi-campaign Asteroseismic Analysis of eight Solar-like pulsating stars observed by the K2 mission
• To be or not to be a black hole: detailed binary population models as a sanity check
• Effects of Winds on the Optical Properties of Type Ib and Ic Supernova Progenitors
• Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
• Regular Radial Velocity Variations in Nine G- and K-type Giant Stars: Eight Planets and One Planet Candidate
• Mass ratio, the hills mechanism, and the galactic centre S-stars
• On the role of reduced wind mass-loss rate in enabling exoplanets to shape planetary nebulae
• Long-rising Type II supernovae resembling supernova 1987A -- I. A comparative study through scaling relations
• Repeated mergers of black hole binaries: implications for GW190521
• SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters
• Can GW231123 have a stellar origin?
• On the origin of the metallicity dependence in dynamically formed extragalactic low-mass X-ray binaries
• Connecting integrated RGB mass loss from asteroseismology and globular clusters
• Mass-loss and composition of wind ejecta in type I X-ray bursts
• The RR Lyrae Delay-Time Distribution: A Novel Perspective on Models of Old Stellar Populations
• Synthesizing Spectra from 3D Radiation Hydrodynamic Models of Massive Stars Using Monte Carlo Radiation Transport
• A rapidly evolving high-amplitude $\delta$ Scuti star crossing the Hertzsprung Gap
• Dust Formation in Common Envelope Binary Interaction -- I: 3D Simulations Using the Bowen Approximation
• Asteroseismic Investigation of 20 Planet and Planet-Candidate Host Stars
• Hot subdwarf B stars with neutron star components II: Binary population synthesis
• Pulsational properties of ten new slowly pulsating B stars
• High Velocity Stars in SDSS/APOGEE DR17
• Deviation of Stellar Orbits from Test Particle Trajectories Around Sgr A* Due to Tides and Winds
• TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence
• Introducing CAFein, a New Computational Tool for Stellar Pulsations and Dynamic Tides
• Dust formation in common envelope binary interactions -- II: 3D simulations with self-consistent dust formation
• SN 2017czd: A Rapidly Evolving Supernova from a Weak Explosion of a Type IIb Supernova Progenitor
• Frequency analysis of KIC 1573174 : shedding light on the nature of HADS stars
• Towards an accurate description of an accretion induced collapse and the associated ejected mass
• KELT-23Ab: A Hot Jupiter Transiting a Near-Solar Twin Close to the TESS and JWST Continuous Viewing Zones
• Whispering in the dark: Faint X-ray emission from black holes with OB star companions
• Unveiling complex magnetic field configurations in red giant stars
• Revised Stellar Parameters for V471 Tau, A Post-common Envelope Binary in the Hyades
• Can friction of the nova envelope account for the extra angular momentum loss in cataclysmic variables?
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• Searching for Anomalies in the ZTF Catalog of Periodic Variable Stars
• The diffusive overshooting approach on Li abundance in clusters
• Pulsations of Pre-White Dwarfs with Hydrogen-dominated Atmospheres
• Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
• Revisiting Orbital Evolution in HAT-P-2 b and Confirmation of HAT-P-2 c
• Evolution of Main-Sequence-like Surviving Companions in Type Ia Supernova Remnants
• Searching for the Next Galactic Luminous Red Nova
• A pre-explosion optical transient event from a white dwarf merger with a giant supernova progenitor
• Constraining the near-core rotation of the gamma Doradus star 43 Cygni using BRITE-Constellation data
• Stellar Shocks From Dark Matter Asteroid Impacts
• Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
• Asteroseismology of main-sequence F stars with \textit{Kepler}: overcoming short mode lifetimes
• SN 2018hna: Adding a Piece to the Puzzles of the Explosion of Blue Supergiants
• Linking the Interiors and Surfaces of Magnetic Stars
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• Dynamical Screening Effects on Big Bang Nucleosynthesis
• Surface structure of 45 Hercules: An otherwise unremarkable Ap star with a surprisingly weak magnetic field
• Dynamical estimate of post main sequence stellar masses in 47 Tucanae
• Unraveling the Formation History of the Black Hole X-ray Binary LMC X-3 from ZAMS to Present
• TIC 278956474: Two close binaries in one young quadruple system, identified by \textit{TESS}
• Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo
• Li-rich and super Li-rich giants produced by element diffusion
• EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope
• The Class of Jsolated Stars and Luminous Planetary Nebulae in old stellar populations
• Orbital Characteristics of the Subdwarf-B and F V Star Binary EC~20117-4014(=V4640 Sgr)
• A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
• The Stability of Massive Main Sequence Stars as a Function of Metallicity
• The APOGEE Library of Infrared SSP Templates (A-LIST): High-Resolution Simple Stellar Population Spectral Models in the H-Band
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Precision Orbit of $\delta$ Delphini and Prospects for Astrometric Detection of Exoplanets
• An evidence-based assumption that helps to reduce the discrepancy between the observed and predicted ${}^7$Be abundances in novae
• Constraining mass transfer and common-envelope physics with post-supernova companion monitoring
• Magnetic Field Evolution of Hot Exoplanets
• Detached and Continuous Circumstellar Matter in Type Ibc Supernovae from Mass Eruption
• The Evolution of Accreting Population III Stars at 10${}^{-6}$-10${}^3$ M${}_{\odot }$/yr
• The Accretion of Solar Material onto White Dwarfs: No Mixing with Core Material Implies that the Mass of the White Dwarf is Increasing
• Models of Metal-Poor Stars with Different Initial Abundances of C, N, O, Mg, and Si. I. Bolometric Corrections Derived from New MARCS Synthetic Spectra and Their Implications for Observed Colour-Magnitude Diagrams
• The Evolution of Population III and Extremely Metal-Poor Binary Stars
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• Re-analysis of the ${}^{24}$Mg($\alpha ,\gamma$)${}^{28}$Si reaction rate at stellar temperatures
• Discrepant Approaches to Modeling Stellar Tides, and the Blurring of Pseudosynchronization
• The Betelgeuse Project II: Asteroseismology
• Mode Mixing and Rotational Splittings: I. Near-Degeneracy Effects Revisited
• Topological modes in stellar oscillations
• Gaia BH1 and BH2 -- evolutionary models with overshooting of the black hole progenitors within the present-day binary separation
• Lithium in red giants: the roles of the He-core flash and the luminosity bump
• Pulsation Analysis of High-Amplitude $\delta$ Scuti Stars with TESS
• Convective overshooting in sdB stars using the $k$-$\omega$ model
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Simulating the tidal disruption of stars by stellar-mass black holes using moving-mesh hydrodynamics
• Detection of ${}^7$Be II in the Classical Nova V5669 Sgr (Nova Sagittarii 2015 No.3)
• Signature of solar g modes in first-order p-mode frequency shifts
• An upper limit on the spins of merging binary black holes formed through binary evolution
• Red supergiant stars in binary systems. I. Identification and characterisation in the Small Magellanic Cloud from the UVIT ultraviolet imaging survey
• Mechanical feedback from black hole accretion as an energy source of core-collapse supernova explosions
• Tidal Dissipation in Evolved Low and Intermediate Mass Stars
• The formation of the magnetic symbiotic star FN Sgr
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• Space Photometry with BRITE-Constellation
• On effects of surface bipolar magnetic regions on the convection zone dynamo
• Comparing Moment-Based and Monte Carlo Methods of Radiation Transport Modeling for Type II-Plateau Supernova Light Curves
• TESS Giants Transiting Giants V -- Two hot Jupiters orbiting red-giant hosts
• Transition of latitudinal differential rotation as a possible cause of weakened magnetic braking of solar-type stars
• Limits on core driven ILOT outbursts of asymptotic giant branch stars
• Gray Radiation Hydrodynamics with the FLASH Code for Astrophysical Applications
• Quantifying How Density Gradients and Front Curvature Affect Carbon Detonation Strength During Type Ia Supernovae
• The Chemical Composition of Extreme-Velocity Stars
• Dipole low-order g mode instability of metal-poor low-mass main-sequence stars due to the $\epsilon$-mechanism
• 4FGL J1120.0-2204: A Unique Gamma-ray Bright Neutron Star Binary with an Extremely Low Mass Proto-White Dwarf
• Photometric Classifications of Evolved Massive Stars: Preparing for the Era of Webb and Roman with Machine Learning
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• The Swan: Data-Driven Inference of Stellar Surface Gravities for Cool Stars from Photometric Light Curves
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• Dust formation and mass loss around intermediate-mass AGB stars with initial metallicity $Z_{\mathrm{ini}}\le 10^{-4}$ in the early Universe I: Effect of surface opacity on the stellar evolution and dust-driven wind
• The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at $\approx$2 AU
• The influence of metallicity on a combined stellar and disk evolution
• Photometric White Dwarf Rotation
• Testing the core overshooting mixing described by the turbulent convection model on the eclipsing binary star HY Vir
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Longitudinally Modulated Dynamo Action in Simulated M-Dwarf Stars
• Standardized Luminosity of the Tip of the Red Giant Branch utilizing Multiple Fields in NGC 4258 and the CATs Algorithm
• Premature Black Hole Death of Population III Stars by Dark Matter
• The YNEV stellar evolution and oscillation code
• Orbital and physical parameters of eclipsing binaries from the ASAS catalogue -- XI. CHIRON investigation of long-period binaries
• Exploring the helium core of the delta Scuti star CoRoT 102749568 with asteroseismology
• NuSTAR bounds on radiatively decaying particles from M82
• Mutual Inclination of Ultra-Short-Period Planets with Time Varying Stellar J2-moment
• Doppler images and the underlying dynamo. The case of AF Leporis
• Revisiting the Red-giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters
• Neural Stellar Population Synthesis Emulator for the DESI PROVABGS
• Discovery, TESS Characterization, and Modeling of Pulsations in the Extremely Low Mass White Dwarf GD 278
• Occultations from an active accretion disk in a 72 day detached post-Algol system detected by K2
• The K2 & TESS Synergy II: Revisiting 26 systems in the TESS Primary Mission
• The Maximum Black Hole Mass at Solar Metallicity
• Exploring the Observability of Surviving Companions of Stripped-Envelope Supernovae: A Case Study of Type Ic SN 2020oi
• Early supernova emission -- logarithmic corrections to the planar phase
• Asteroseismology of RRab variable star EZ Cnc from K2 photometry and LAMOST spectroscopy
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• An unsupervised method for identifying $X$-enriched stars directly from spectra: Li in LAMOST
• Constraining white dwarf structure and neutrino physics in 47 Tucanae
• Enhanced production of 60Fe in massive stars
• Measurement of the ${}^{159}$Tb(n, $\gamma$) cross section at the CSNS Back-n facility
• Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses
• Nonlinear Mixed Modes in Red Giants
• Precise Evolutionary Asteroseismology of High-Amplitude δ Scuti Star AE Ursae Majoris
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• Search for ${}^{22}$Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes
• A discontinuity in the luminosity-mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The eclipsing binary HD 185912
• Flares on A-type stars: Evidence for heating of solar corona by nanoflares?
• WIYN Open Cluster Study. XC. Radial-velocity Measurements and Spectroscopic Binary Orbits in the Open Cluster NGC 2506
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• The Pre-main Sequence: Challenges and Prospects for Asteroseismology
• Origin and Evolution of Angular Momentum of Class II Disks
• Characterising abundance-age relations of GALAH stars using oxygen-enhanced stellar models
• Dynamical parallax, physical parameters and evolutionary status of the components of the bright eclipsing binary α Draconis
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Occurrence rate of hot Jupiters orbiting red giant stars
• Stellar Helium Burning in Other Universes: A solution to the triple alpha fine-tuning problem
• Rotational splitting and asteroseismic modelling of the delta Scuti star EE Camelopardalis
• Discovery of a young pre-intermediate polar
• Evolutionary and Observational Consequences of Dyson Sphere Feedback
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
• Red giants evolutionary status determination: the complete Kepler catalog
• On asymmetric dark matter constraints from the asteroseismology of a subgiant star
• Absolute dimensions and apsidal motion of the eclipsing binaries V889 Aql and V402 Lac
• Effects of the core-collapse supernova ejecta impact on a rapidly rotating massive companion star
• Universes without the Weak Force: Astrophysical Processes with Stable Neutrons
• One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors
• VLT/X-shooter spectroscopy of massive young stellar objects in the 30 Doradus region of the Large Magellanic Cloud
• Frequency identification and asteroseismic analysis of the red giant KIC 9145955: fundamental parameters and helium core size
• Tidally excited oscillations in hot white dwarfs
• Differentiating Formation Models with New Dynamical Masses for the PDS 70 Protoplanets
• TOI-4504: Exceptionally large Transit Timing Variations induced by two resonant warm gas giants in a three planet system
• MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation
• The composition of massive white dwarfs and their dependence on the C-burning modeling
• The Impacts of Neutron-Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison
• Orbital Dynamics and the Evolution of Planetary Habitability in the AU Mic System
• A search for transit timing variations in the HATS-18 planetary system
• Fully Nonadiabatic Analysis of Vibrational Instability of Population III Stars due to the $\epsilon$-Mechanism
• The Influence of Disk Composition on the Evolution of Stars in the Disks of Active Galactic Nuclei
• Magnetic Inclination Evolution of Accreting Neutron Stars in Intermediate/Low-Mass X-ray Binaries
• BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Rotational Variation Allows for Narrow Age Spread in the Extended Main Sequence Turnoff of Massive Cluster NGC 1846
• Towards early-type eclipsing binaries as extragalactic milestones: II. NLTE spectral analysis and stellar parameters of the detached O-type system OGLE-LMC-ECL-06782 in the LMC
• XO-7 b: A transiting hot Jupiter with a massive companion on a wide orbit
• Polygram Stars: Resonant Tidal Excitation of Fundamental Oscillation Modes in Asynchronous Stellar Coalescence
• Elimination of the Blue Loops in the Evolution of Intermediate-mass Stars by the Neutrino Magnetic Moment and Large Extra Dimensions
• Gravitational Wave Heating of Stars and Accretion Disks
• Shadows of our Former Companions: How the Single-Degenerate Binary Type Ia Supernova Scenario Affects Remnants
• A closer look at the $pp$-chain reaction in the Sun: Constraining the coupling of light mediators to protons
• Quantum effects on plasma screening for thermonuclear reactions in laser-generated plasmas
• A multiphase study of theoretical and observed light curves of classical Cepheids in the Magellanic Clouds
• The Formation of Bimodal Dust Species in Nova Ejecta I: Chemical Conditions
• The near-core rotation of HD 112429: a gamma Doradus star with TESS photometry and legacy spectroscopy
• A Framework for Relative Biosignature Yields from Future Direct Imaging Missions
• The Betelgeuse Project III: Merger Characteristics
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• The young stellar content of the giant HII regions M8, G333.6-0.2, and NGC6357 with VLT/KMOS
• Evolutionary Constraints on the Long-period Subdwarf B Binary PG 1018-047
• Numerical Modelling of Tertiary Tides
• Inferring the progenitor mass-kinetic energy relation of stripped-envelope core-collapse supernovae from nebular spectroscopy
• Unresolved Rossby and gravity modes in 214 A and F stars showing rotational modulation
• Convection physics and tidal synchronization of the subdwarf binary NY Virginis
• A transiting giant planet in orbit around a 0.2-solar-mass host star
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. III. HD 8374 and HD 24546
• The future influence of six exoplanets on the envelope properties of their parent stars on the giant branches
• Optical Appearance of Eccentric Tidal Disruption Events
• The binary evolution of SAX J1808.4-3658: Implications of an evolved donor star
• Type IIP Supernova Progenitors III: Blue to Red Supergiant Ratio in Low Metallicity Models with Convective Overshoot
• Photodynamical Modeling of the Fascinating Eclipses in the Triple-Star System KOI-126
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• Stellar winds near massive black holes: The case of the S-stars
• A close-in puffy Neptune with hidden friends: The enigma of TOI 620
• Populations of Neutron Star Ultraluminous X-ray Sources: Mind your b's and B's
• A Holistic and Probabilistic Approach to the Ground-based Data of HAT-P-19 System
• Ionising Feedback Effects on Star Formation in Globular Clusters with Multiple Stellar Populations
• Unraveling the origin of giant exoplanets: Observational implications of convective mixing
• Heavy Dark Matter in White Dwarfs: Multiple-Scattering Capture and Thermalization
• Simulating a stellar contact binary merger -- I. Stellar models
• A binary with a $\delta$~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821
• Radio Transients from Newborn Black Holes
• Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
• Revising Properties of Planet-host Binary Systems I.: Methods and Pilot Study
• Detached Eclipsing Binaries in Compact Hierarchical Triples: Triple-lined systems BD+44 2258 and KIC 06525196
• Distorted surfaces of magnetic helium-peculiar stars: An application to a Cen
• Peeking beneath the precision floor -- II. Probing the chemo-dynamical histories of the potential globular cluster siblings, NGC 288 and NGC 362
• Apsidal motion and a light curve solution for thirteen LMC eccentric eclipsing binaries
• Young Stars near Cometary Globule CG 30 in the Tumultuous Gum Nebula
• Magnetic Archaeology of Early-Type Stellar Dynamos
• Measuring solar neutrinos over Gigayear timescales with Paleo Detectors
• Simulating the deposition of angular momentum by jets in common envelope evolution
• Refractory and Volatile Species in the UV-to-IR Transmission Spectrum of Ultra-hot Jupiter WASP-178b with HST and JWST
• Type Ia Supernova Explosions from Hybrid Carbon-Oxygen-Neon White Dwarf Progenitors That Have Mixed During Cooling
• Evolution of Rotating 25 M${}_{\odot }$ Population III star: Physical Properties and Resulting Supernovae
• Novae: An Important Source of Lithium in the Galaxy
• Period Change Rates of Large Magellanic Cloud Cepheids using MESA
• Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri
• Stability Analysis of Strange-Modes in Hot Massive Stars with Time-Dependent Convection
• Leveraging HST with MUSE: II. Na-abundance variations in intermediate age star clusters
• Neutrino Emissivities as a Probe of the Internal Magnetic Fields of White Dwarfs
• When does the onset of multiple stellar populations in star clusters occur-II: No evidence of multiple stellar populations in Lindsay 113
• Pulsational Pair-instability Supernovae. II. Neutrino Signals from Pulsations and their Detection by Terrestrial Neutrino Detectors
• Linear dust polarization during the embedded phase of protostar formation
• Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
• He abundance of Dense Circumstellar Clumps in the Cassiopeia A Supernova Remnant
• Uncovering the chemical structure of the pulsating low-mass white dwarf SDSS J115219.99+024814.4
• Scalable stellar evolution forecasting: Deep learning emulation vs. hierarchical nearest neighbor interpolation
• A low-mass companion desert among intermediate-mass visual binaries: The scaled-up counterpart to the brown dwarf desert
• The effect of aspherical stellar wind of giant stars on the symbiotic channel of type Ia supernovae
• Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328
• High mass X-ray binaries as progenitors of gravitational wave sources
• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• SN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovae
• Optical and Near-Infrared Excesses are Correlated in T Tauri Stars
• Direct Measurement of Astrophysically Important Resonances in ${}^{38}\mathrm{K}(p,\gamma ){}^{39}\mathrm{Ca}$
• Searching for solar-like oscillations in pre-main sequence stars using APOLLO
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Close encounters of black hole - star binaries with stellar-mass black holes
• Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main sequence stars
• Seismic characterization of red giants going through the Helium-core flash
• Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts
• Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries
• Optical color of Type Ib and Ic supernovae and implications for their progenitors
• TOI-712: a system of adolescent mini-Neptunes extending to the habitable zone
• Testing tidal theory using Gaia binaries: the red giant branch
• Analytic approximations for massive close post-mass transfer binary systems
• ZZ Ceti stars of the southern ecliptic hemisphere re-observed by TESS
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
• The Effects of Metallicity on Convective Overshoot Behaviour in Models of delta Scuti Variable Stars
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
• A dearth of close-in planets around rapidly rotating stars or a dearth of data?
• An Ultraviolet-Optical Color-Metallicity relation for Red Clump Stars using GALEX and Gaia
• Unveiling the nitrogen-rich massive star in the metal-poor galaxy NGC 4068
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• GABE: Galaxy Assembly with Binary Evolution
• Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures
• Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
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• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
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• Minimum Orbital Periods of H-Rich Bodies
• X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
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• Impact of central mixing scheme and nuclear reaction network on the extent of convective cores
• Gaia DR2 giants in the Galactic dust -- II. Application of the reddening maps and models
• Modelling stars with Gaussian Process Regression: Augmenting Stellar Model Grid
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• Probing red-supergiant atmospheres and winds with early-time high-cadence high-resolution type II supernova spectra
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• Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692
• Comprehensive Bayesian Modeling of Tidal Circularization in Open Cluster Binaries part I: M 35, NGC 6819, NGC 188
• Dark Matter-Induced Baryonic Feedback in Galaxies
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• The preliminary statistical analysis of LAMOST DR8 low resolution AFGK stars
• The ESO UVES/FEROS Large Programs of TESS OB pulsators. II. On the physical origin of macroturbulence
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• The Sun: Light Dark Matter and Sterile Neutrinos
• Oscillations of red giant stars with magnetic damping in the core. I. Dissipation of mode energy in dipole-like magnetic fields
• HIP 15429: A newborn Be star on an eccentric binary orbit
• Magnetic Webs in Stellar Radiative Zones
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• Microlensing at Cosmological Distances: Event Rate Predictions in the Warhol Arc of MACS 0416
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• Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests
• Two-Dimensional Radiation-Hydrodynamic Simulations of Luminous Red Novae
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• Circumstellar CO J = 3-2 detected around the evolving metal-poor ([Fe/H] ~ -1.15 dex) AGB star RU Vulpeculae
• The Formation of Bimodal Dust Species in Nova Ejecta
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• Type IIP Supernova Progenitors II: Stellar Mass and Obscuration by the Dust in the Circumstellar Medium
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• Zahn's Theory of Dynamical Tides and Its Application to Stars
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• Reinterpreting the Polluted White Dwarf SDSS J122859.93+104032.9 in Light of Thermohaline Mixing Models: More Polluting Material from a Larger Orbiting Solid Body
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• Astrophysical Parameter Inference on Accreting White Dwarf Binaries using Gravitational Waves
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• On the rapid orbital expansion in the compact low-mass X-ray binary 2A 1822$-$371
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• A Photometric, Spectroscopic, and Apsidal Motion Analysis of the F-type Eclipsing Binary BW Aquarii from K2 Campaign 3
• Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
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• Abundance Pattern Fitting with Bayesian Inference: Constraining First Stars' Properties and Their Explosion Mechanism with Extremely Metal-poor Stars
• Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars
• Asteroseismology of the pre-main-sequence $\delta$ Scuti pulsator IP Persei
• Rapid expansion of red giant stars during core helium flash by waves propagation to the envelope and implications to exoplanets
• In search of gravity mode signatures in main sequence solar-type stars observed by Kepler
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra
• Searching for compact objects in the single-lined spectroscopic binaries of the young Galactic cluster NGC 6231
• Angular momentum fluxes caused by Lambda-effect and meridional circulation structure of the Sun
• KIC 12268220: A $\delta$ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System
• Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers
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• Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae
• Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
• Spatio-temporal non-localities in a solar-like mean-field dynamo
• Suggested magnetic braking prescription derived from field complexity fails to reproduce the cataclysmic variable orbital period gap
• Red giant - jet collisions in galactic nuclei I: 3D hydrodynamical model of a few stellar orbits
• Dark Matter Mini-halo around the Compact Objects: the Formation, Evolution and Possible Contribution to the Cosmic Ray Electrons/Positrons
• Effect of Binary Fraction on Horizontal Branch Morphology under Tidally Enhanced Stellar Wind
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• The effects of Thomson scattering and chemical mixing on early-time light curves of double peaked type IIb supernovae
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• Mixed-mode coupling in the Red Clump I. Standard single star models
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• Migration and Evolution of giant ExoPlanets (MEEP) II: Super-Jupiters and Lithium-rich Host Stars
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• HD 42477: coupled r modes, g modes and a p mode in an A0Vnne star
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• Lazarus Stars: Numerical investigations of stellar evolution with star-lifting as a life extension strategy
• Neutrino flavour as a test of the explosion mechanism of core-collapse supernovae
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• Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores
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• Mode Angular Degree Identification in Subgiant Stars with Convolutional Neural Networks based on Power Spectrum
• Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor
• Magnetic Fields or Overstable Convective Modes in HR 7495: Exploring the Underlying Causes of the Spike in the 'Hump & Spike' Features
• On the behaviour of spin-orbit connection of exoplanets
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• Silicon Isotopic Composition of Mainstream Presolar SiC Grains Revisited: The Impact of Nuclear Reaction Rate Uncertainties
• Stellar rotation and its connection to the evolution of hydrogen-dominated atmospheres of exoplanets
• Asteroseismology: Looking for axions in the red supergiant star Alpha Ori
• The effect of stellar evolution on dispersal of protoplanetary disks: Disk fraction in star-forming regions
• A rapidly fading star as a type II obscuring intermediate luminosity optical transient (ILOT) in a triple star system
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• Constraining Accreted Neutron Star Crust Shallow Heating with the Inferred Depth of Carbon Ignition in X-ray Superbursts
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215.82+111745.0: a model with $p$-mode pulsations consistent with the observations
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• The evolutionary status of chemically peculiar eclipsing binary star DV Boo
• Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
• The Environments around W Serpentis Systems: Independent Limits on System Masses and Extended Envelopes
• Exploring the internal rotation of the extremely low-mass He-core white dwarf GD 278 with TESS asteroseismology
• Everything that glitters is not gold: V1315 Cas is not a dormant black hole
• A study on missing lines in the synthetic solar spectrum near the Ca triplet
• Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
• Dynamos and Differential Rotation: Advances at the Crossroads of Analytics, Numerics, and Observations
• Absolute dimensions of the F-type eclipsing binary V2154 Cygni
• Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
• Digital Infrastructure in Astrophysics
• Wave-Driven Mixing Enhanced by Rotation in Red Giant Branch Stars
• Impact of Asymmetrical Mass Ejection from Proto-White Dwarfs on the Properties of Binary Millisecond Pulsars
• On the Geometry of the Near-Core Magnetic Field in Massive Stars
• An irradiated-Jupiter analogue hotter than the Sun
• Off-centre convective zones in mass accreting stellar models
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Seismology and diffusion of ultramassive white dwarf magnetic fields
• Analyses of Hydrogen-stripped core-collapse supernovae using MOSFiT and MESA based tools
• A Trio of Giant Planets Orbiting Evolved Star HD 184010
• Narrow absorption lines from intervening material in supernovae. II. Galaxy properties
• Exploring the small-scale magnetic fields of the solar analog KIC 8006161 using asteroseismology
• On the effect of pulsar evaporation on the cooling of white dwarfs
• Radiative acceleration calculation methods and abundance anomalies in Am stars
• Twenty-three New Heartbeat Star Systems Discovered Based on TESS Data
• Pulsations driven by the $\epsilon$-mechanism in post-merger remnants: first results
• Accretion of Planetary Material onto Host Stars
• Evolution and period change in RR Lyr variables of the globular cluster M 3
• Study with WhoSGlAd of the acoustic depth of the helium glitch across the seismic HR diagram and its impact on the inferred helium abundance
• A Close-in Planet Orbiting Giant Star HD 167768
• Neutrinos and Asteroseismology of Stars over the Helium Flash
• Off-centre ignition of sub-Chandrasekhar white dwarfs does not resolve the tension with the observed $t_0$-$M_{\mathrm{Ni}56}$ relation of type Ia supernovae
• Where to find over-massive brown dwarfs: new benchmark systems for binary evolution
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
• Binary Stars Approaching Supermassive Black Holes: Hydrodynamics of Stellar Collisions, Mass Fallback and Partial TDEs
• Conservative Initial Mapping For Multidimensional Simulations of Stellar Explosions
• Ocean g-modes on transient neutron stars
• The shape of convection in 2D and 3D global simulations of stellar interiors
• HATS-34b and HATS-46b: Re-characterisation Using TESS and Gaia
• White dwarf eccentricity fluctuation and dissipation by AGB convection
• MESA-QUEST: Modeling Quasi-Stars in MESA
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Millions of Main-Sequence Binary Stars from Gaia BP/RP Spectra
• K2 Observations of 95 Vir: delta Scuti Pulsations in a Chromospherically Active Star
• Hydrodynamic 3D Simulation of Roche Lobe Overflow in High-mass X-Ray Binaries
• On rare core collapse supernovae inside planetary nebulae
• Supernovae at the cosmic dawn
• The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars
• Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology
• Emulators for stellar profiles in binary population modeling
• Nonlinear tidal excitation of super-harmonic gravity waves in main-sequence stars in binary and exoplanetary systems
• Asteroseismology of the DBV star CBS 114
• Drawing the line between explosion and collapse in electron-capture supernovae -- I. Impact of conductive flame speeds and ignition conditions on the explosion mechanism
• The frequency by mass of Galactic carbon stars inferred from Gaia measurements of star cluster members
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Ultrashort-period WD binaries are not undergoing strong tidal heating
• Beyond binarity in A stars II. Disentangling the four stars in the vicinity of the triple HIP 87813 within the quintuple system HJ2814
• Empirical Relations for the Sensitivities of Solar-like Oscillations to Magnetic Perturbations
• Seismic detection of core magnetic fields in red giants using the gravity offset
• The rotational shear in pre-collapse cores of massive stars
• A Search For Pulsations in the Optical Light Curve of the Nova ASASSN-17hx
• Core-collapse supernova from a possible progenitor star of 100 M${}_{\odot }$
• The K2 Galactic Archaeology Program: Overview, target selection and survey properties
• Constraining Axions with ZTF J1901+1458
• Absolute dimensions of the early F-type eclipsing binary V506 Ophiuchi
• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
• Asteroseismology and Buoyancy Glitch Inversion with Fourier Spectra of Gravity Mode Period Spacings
• The Signature of a Windy Radio Supernova Progenitor in a Binary System
• A model of the Mira-type star T UMi
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Planetary Dynamos in Evolving Cold Gas Giants
• A uvbyCaHbeta CCD Analysis of the Open Cluster Standard, M67,and its Relation to NGC 752
• Rotationally and tidally distorted compact stars A theoretical approach to the gravity-darkening exponents for white dwarfs
• Three-component Phase Separation for Ultramassive White Dwarf Models
• Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA
• Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
• Solar models with protosolar accretion and turbulent mixing
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Constraining the Rotation Profile in a Low-Luminosity Subgiant with a Surface Rotation Measurement
• Searching for Galactic Red Supergiants with Gaia RVS Spectra
• Testing the sources of the peculiar abundances in globular clusters
• Beyond the Nyquist frequency: Asteroseismic catalog of undersampled Kepler late subgiants and early red giants
• A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters
• Discovery of a Highly Eccentric, Chromospherically Active Binary: ASASSN-V J192114.84+624950.8
• An Analytic, Fully Relativistic Framework for Tidal Disruption Event Streams in Schwarzschild Geometry
• Collision of Two Stellar Associations in the Nearby Gum Nebula
• Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors
• The Energy Sharing Timescale in an Analytic Framework for Common Envelope Hydrodynamics
• A stringent upper limit on Be star fractions produced by binary interaction
• Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation
• The SDSS-HET Survey of Kepler Eclipsing Binaries. A Sample of Four Benchmark Binaries
• Spectroscopy of the massive interacting binary UU Cassiopeiae
• Chemical abundances and doppler imaging of the Ap Si/He-wk star HD 100357
• Jet-driven active galactic nucleus feedback in galaxy formation before black hole formation
• Magellanic System Stars Identified in SMACS J0723.3-7327 James Webb Space Telescope Early Release Observations Images
• Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
• Asteroseismology of low-mass stars: the balance between partial ionisation and Coulomb interactions
• Impact of Simultaneous Stellar Modeling Uncertainties on the Tip of the Red Giant Branch for Axion-Election Coupling
• Merged white dwarfs and nucleosynthesis
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Analysis of accretion disc structure and stability using open code for vertical structure
• Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729
• A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054
• Unequivocal detection of the tidal deformation of a red giant in a binary system via interferometry
• V2368 Oph: An eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Oph
• Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
• Asteroseismology of sz lyn using multi-band high time resolution photometry from ground and space
• The depletion of the red supergiant envelope radiative zone during common envelope evolution
• Modeling the emission lines from r-process elements in Supernova nebulae
• 3D non-LTE Ca II line formation in metal-poor FGK stars. I. Abundance corrections, radial velocity corrections, and synthetic spectra
• Abundance Uncertainties Obtained With the PizBuin Framework For Monte Carlo Reaction Rate Variations
• ${\tau }^9$ Eri: A bright pulsating magnetic Bp star in a 5.95-day double-lined spectroscopic binary
• Searching for Low-mass Population III Stars Disguised as White Dwarfs
• A post-common-envelope binary with double-peaked Balmer emission lines from TMTS
• Probing the Axion-Nucleon Coupling with Supergiant Stars
• Pre-Supernova (Anti)Neutrino Emission Due to Weak-Interaction Reactions with Hot Nuclei
• Magnetic dynamos powered by white dwarf superficial convection
• A Continuous Galactic Line Source of Axions: The Remarkable Case of 23Na
• Calibration of Binary Population Synthesis Models Using White Dwarf Binaries from APOGEE, GALEX and Gaia
• The rate of period change in DAV stars
• Application of a screened Coulomb potential in fitting the DAV star HS 0507+0434B
• A solution to the tension of burning on neutron stars and nuclear physics
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Asteroseismic modelling of the Binary HD 176465
• Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars
• Study of the effects of magnetic braking on the lithium abundances of the Sun and solar-type stars
• Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• Extraction of Physical Parameters of RRab Variables using Neural Network based Interpolator
• Under an Iron Sky: On the Entropy at the Start of the Universe
• Evolution of a Long-Lived Deep-Seated Main-Sequence Magnetic Field During White Dwarf Cooling
• Explosions of pulsating red supergiants: a natural pathway for the diversity of Type II-P/L supernovae
• Multiple stellar populations at less evolved stages-III: a possible helium spread in NGC 2210
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• The dispersion of period spacing for DAV stars
• Irradiation effect and binary radio pulsars with giant companions
• Good things come to those who wait: Watching donor stars evolve towards a mass-transfer instability
• Helium enrichment during classical nova outbursts
• Onset of common envelope evolution during a core helium flash by rapid envelope expansion
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Star Formation for Predictive Primordial Galaxy Formation
• Light Axion Emission and the Formation of Merging Binary Black Holes
• The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations
• Engulfment of a hot Jupiter as a possible origin of the rapid spin and internal spin misalignment of the planet-hosting red giant Kepler-56
• The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf's code predictions
• Identification and characterization of optical companions to the population of millisecond pulsars in the globular cluster M3
• The detached, evolved post-mass-exchange binary V643 Orionis
• Influence of irradiation-driven winds on the evolution of intermediate-mass black hole X-ray binaries
• Spectral Energy Distribution of the First Galaxies: Contribution from Pre-Main-Sequence Stars
• Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
• Dynamical mass of a solar-like oscillator at the main-sequence turnoff from Gaia astrometry & ground-based spectroscopy
• From Main Sequence Binary to Blast: MESA Modeling of the Double-Detonation Progenitor PTF1~J2238+7430
• Wide sdB binaries. I. Orbital and atmospheric parameters
• Toward a Comprehensive Grid of Cepheid Models with MESA II. Impact of Physical and Numerical Assumptions on Elemental Abundances
• Discovery of Galactic center ejected star in DESI DR1
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• The Onset of Convective Coupling and Freezing in the White Dwarfs of 47 Tucanae
• Foam: A Python package for forward asteroseismic modelling of gravity modes
• Stellar response after stripping as a model for common-envelope outcomes
• An Alternative Formation Scenario for Uranium-rich Giants: Engulfing a Earth-like Planet
• Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
• The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars
• Magnetized oscillatory double-diffusive convection
• Partial, zombie, and full tidal disruption of stars by supermassive black holes
• Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Accreting White Dwarfs: Effect of WD Composition on Helium Ignition During Slow Accretion
• On the parallelization of stellar evolution codes
• Chemically peculiar stars on the pre-main sequence
• Type Ia Supernovae from First-generation Stars
• Second-generation planet formation after tidal disruption from common envelope evolution
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• Meridional Circulation Streamlined
• The response of a red supergiant to a common envelope jets supernova (CEJSN) impostor event
• CY Aquarii: A Triple System with Twin Companions
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• Violent mergers revisited: The origin of the fastest stars in the Galaxy
• Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint
• GD 99: Re-investigation of an old ZZ Ceti companion
• Modeling Atmospheric Ion Escape from Kepler-1649 b and c over Time
• Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• Stellar Wind -- Magnetosphere Interactions in Hot Jupiters
• The influence of rotation and metallicity on the explodability of massive stars
• Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
• Double-faced white dwarfs and the magnetic inhibition of convection
• 3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors
• Exploring the physical properties of the $\gamma$ Dor binary star RX Dra with photometry and asteroseismology
• Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts
• Probing the internal magnetism of stars using asymptotic magneto-asteroseismology
• Light Curve Models of Convective Common Envelopes
• Discovery of a Short Period Pulsator from Istanbul University Observatory
• Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
• Can circumstellar interaction explain the strange light curve features of Type Ib/c supernovae?
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Advancing Globular Cluster Constraints on the Axion-Photon Coupling
• Asteroseismology of the DOV star PG 1159-035
• Dynamical Mass Loss at the End of TP-AGB stars
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• The AGB bump: a calibrator for the core mixing
• Evolution and Explosion of Massive Stars Leading to IIP-IIL SNe with MESA and SNEC
• Asymptotic power spectra and visibilities of damped mixed modes
• Slow White Dwarf Mergers as a New Galactic Source of Trans-Iron Elements
• Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission
• Sub-photospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves
• Discovery of a runaway star likely ejected by a Type Iax Supernova
• A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
• Blue Loops, Cepheids, and Forays into Axions
• A distant brown dwarf coplanar to a warm Jupiter and a hot super-Earth
• Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects
• Near-critical magnetic fields in Kepler red giants
• Icy Volatile Enhancements in Evolving Protoplanetary Disks
• Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
• Analysis of strange-mode instability with time-dependent convection in hot massive stars
• Simulating super-Chandrasekhar white dwarfs
• Analysis of TESS field eclipsing binary star V948 Her: a pulsating or non-pulsating star?
• Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
• Asteroseismology of red giants & galactic archaeology
• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• A 3D model for the stellar populations in the nuclei of NGC 1433,NGC 1566, and NGC 1808
• Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
• Exploring the Small-scale Magnetic Fields in the Atmosphere of HD 49385 by Asteroseismic Analysis
• Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
• Core-envelope coupling of gravito-inertial waves in pre-main-sequence solar-type stars
• Gaia-GIC-1: An Evolving Catastrophic Planetesimal Collision Candidate
• Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids
• NGC 1850 BH1 is another stripped-star binary masquerading as a black hole
• Accretion induced merger leading to core collapse supernovae in old stellar populations
• Patchy nightside clouds on ultra-hot Jupiters: General Circulation Model simulations with radiatively active cloud tracers
• Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
• Seismic and spectroscopic analysis of 9 bright red giants observed by Kepler
• A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
• Measuring Dust Masses of Protoplanetary Disks in Serpens and L1641/L1647 with ALMA
• $\delta$ Circini: A massive hierarchical triple system with an eclipsing binary
• Ancient, eclipsing, tidally-locked: A blue lurker progenitor in the population of extreme-velocity star candidates
• Evolved eclipsing binary systems in the Galactic bulge: Precise physical and orbital parameters of OGLE-BLG-ECL-305487 and OGLE-BLG-ECL-116218
• The evolutionary history of ultra-compact accreting binaries. I. Chemical abundances and formation channel of the eclipsing AM CVn system ZTF J225237.05-051917.4 from HST spectroscopy
• High-resolution spectroscopy of detached eclipsing binaries during total eclipses
• A new sample of massive B-type contact binary candidates from the OGLE survey of the Magellanic Clouds
• Observational Properties of $\beta$ Cephei Stars: 88 new samples discovered Based on TESS and Gaia Data
• Empirical instability strip for classical Cepheids II. The Small Magellanic Cloud galaxy
• Entering the Wind Roche Lobe Overflow realm in Symbiotic Systems
• Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• A Lagrangian construction of rotating stars
• Relativistic Coulomb Screening in Pulsational Pair Instability Supernovae
• Nuclear data activities for medium mass and heavy nuclei at Los Alamos
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
• Two unseen massive white dwarf candidates in close binaries
• The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
• Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri
• Asteroseismic Constraints on the Models of Hot B Subdwarfs: Convective Helium-Burning Cores
• Insights from Asteroseismology of Massive Stars: The Need for Additional Angular Momentum Transport Mechanisms
• On the non-dissipative orbital evolution of a binary system comprising non-compact components with misaligned spin and orbital angular momenta
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• Critical Metallicity of Cool Supergiant Formation. II. Physical Origin
• Rare events of a peculiar thermonuclear supernova that precedes a core collapse supernova
• Probing high-mass stellar evolutionary models with binary stars
• On the nature of the candidate T-Tauri star V501 Aurigae
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Neutrinos from stars in the Milky Way
• Spectroscopic and asteroseismic analysis of the secondary clump red giant HD 226808
• Ultra-compact X-ray binaries with high luminosity: a key for a new scenario
• Discerning internal conditions of pulsating hot subdwarf B stars. Modelling multiple trapped modes in KIC 10001893
• Tidal capture and repeating partial tidal disruption events of giant stars
• Kinematics of B-F Stars as a Function of Their Dereddened Color from Gaia and PCRV Data
• A database of spectral energy distributions of progenitors of core-collapse supernovae
• Inflated Eccentric Migration of evolving gas giants II: Numerical methodology and basic concepts
• Urca Nuclide Production in Type-I X-ray Bursts and Implications for Nuclear Physics Studies
• A transiting hot Jupiter with two outer siblings orbiting an intermediate-mass post main-sequence star
• Atmospheric mass loss and stellar wind effects in young and old systems II: Is TOI-942 the past of TOI-421 system?
• Impacts of nuclear-physics uncertainty in stellar temperatures on the s-process nucleosynthesis
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
• Cyclic light variations and accretion disk evolution in the LMC eclipsing binary OGLE-LMC-DPV-062
• Huntsman may need to be irradiated
• Eighteen Exoplanet Host Stars from the NPOI Data Archive
• Primordial black holes capture by stars and induced collapse to low-mass stellar black holes
• Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
• The COMBS Survey -- III. The Chemodynamical Origins of Metal-Poor Bulge Stars
• Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid
• Isotopic Compositions of Ruthenium Predicted from the NuGrid Project
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Detectability of compact intermediate-mass black hole binaries as low-frequency gravitational wave sources: the influence of dynamical friction of dark matter
• Pulsations of blue supergiants before and after helium core ignition
• Jsolated Stars of Low Metallicity
• Vibrational Instability of Metal-Poor Low-Mass Main-Sequence Stars
• Modelling differential rotation of red giants: the case of the evolved sun
• PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators
• A Theoretical Study of the Structure and Elemental Abundances of HD 20794
• Convective Penetration in Early-Type Stars
• Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
• Gravitational-Wave Signatures of Massive Black Hole Formation
• A Multi-Planet System's Sole Super-Puff: Exploring Allowable Physical Parameters for the Cold Super-Puff HIP 41378 f
• The bimodal distribution of donor stars in X-ray binaries
• The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars
• A Black Hole is Born: 3D GRMHD Simulation of Black Hole Formation from Core-Collapse
• HIP 67506 C: MagAO-X Confirmation of a New Low-Mass Stellar Companion to HIP 67506 A
• Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss
• Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
• Magellan/IMACS spectroscopy of Grus I: A low metallicity ultra-faint dwarf galaxy
• Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Mechanisms for magnetic braking boost and disruption: the role of irradiation-driven winds and convective turnover time spike in cataclysmic variables
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution
• Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
• Viscous and centrifugal instabilities of massive stars
• Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2
• Pre-main sequence evolution of low-mass stars in Eddington-inspired Born-Infeld gravity
• High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• Eccentricities of millisecond pulsars with intermediate-mass progenitors
• The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
• Validation of the Gaia Early Data Release 3 parallax zero-point model with asteroseismology
• The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
• Faint intermediate luminosity optical transients (ILOTs) from engulfing exoplanets on the Hertzsprung gap
• A search for transits among the δ Scuti variables in Kepler
• The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• Detached Shell Carbon Stars: Tracing Thermal Pulses on the Asymptotic Giant Branch
• Asteroseismic Analysis of a Red Giant KIC 9145955 by Including the Small-scale Magnetic Fields in the Atmosphere
• Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• Chemical fingerprints of binary mass transfer in massive stars
• Radio observations of massive stars in the Galactic centre: The Quintuplet cluster
• Inactive longitude and superflare in the active single-lined pre-main sequence binary V2279 Cyg
• OO Dra: an Algol-type binary formed through an extremely helium-poor mass accretion revealed by asteroseismology
• Peculiarity of the stellar CNO cycle with energetic particles
• A magnetic field detection in the massive O-type bright giant 63 Oph
• Stellar ${\beta }^{-}$-decay rate of ${}^{63}$Ni and its impact on the $s$-process nucleosynthesis in massive stars
• Detailed Characterization of Heartbeat Stars and their Tidally Excited Oscillations
• The final fates of close hot subdwarf - white dwarf binaries: mergers involving He/C/O white dwarfs and the formation of unusual giant stars with C/O-dominated envelopes
• Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
• Precise physical parameters of three late-type eclipsing binary giant stars in the Large Magellanic Cloud
• Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• The reason for the occurrence of W-type contact binaries
• Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network
• JWST observations of 47 Tucanae: I. The low-mass main sequence down to the hydrogen-burning limit
• Evolution of the ZTF SLRN-2020 star-planet merger
• Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption
• Asteroseismic Diagnostics for Semi-Convection in B Stars in the Era of K2
• A New Versatile Code for Gamma-Ray Monte-Carlo Radiative Transfer
• Can the Anomalous Magnetic Braking of Ap/Bp Stars Explain the Orbital Decay of Algol-type Binaries?
• Damping of Oscillations in Red Giants by Resonant Mode Coupling
• TYC~2990-127-1: an Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer
• Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA
• Planetary migration in wind-fed non-stationary accretion disks in binary systems
• Apsidal motion and proximity effects in the massive binary BD+60 497
• Expectation for the MeV Gamma-Ray Emission from Pair-Instability Supernovae
• StelNet: Hierarchical Neural Network for Automatic Inference in Stellar Characterization
• Physical interpretation of the oscillation spectrum on the RGB and AGB
• Ensemble seismic study of the properties of the core of Red Clump stars
• BVRI Photometric Observations, Light Curve Solutions and Orbital Period Analysis of BF Pav
• Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
• Attempting an accurate age estimate of the open cluster NGC 6633 using CoRoT and Gaia
• The Cooling of Old White Dwarfs in 47 Tucanae
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Absolute physical parameters of three poorly studied detached eclipsing binaries
• Formation, diffusion and accreting pollution of DB white dwarfs
• A Warm Massive Pair of Planets around TOI-1232 Revealed with Transit-timing Variations and Doppler Spectroscopy
• Fast giant flares in discs around supermassive black holes
• Stationary accretion flow with nuclear burning
• Possible in situ formation of Uranus and Neptune via Pebble Accretion
• Can small-scale magnetic fields be the major cause for the near-surface effect of the solar p-mode frequencies?
• Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties
• Formation of black holes from He stars
• A hybrid SLAM-Payne framework for atmospheric parameter and abundance determination of early-type Stars from LAMOST DR9 low-resolution Spectra
• The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars
• Three-dimensional simulations of accretion disks in pre-CE systems
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• Heavy dark matter in rapidly evolving massive stars
• Potential Habitability as a Stellar Property: Effects of Model Uncertainties and Measurement Precision
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
• Resolution Study of Thermonuclear Initiation in White Dwarf Tidal Disruption Events
• Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
• Star formation in two irradiated globules around Cygnus OB2
• Revisiting the Evolutionary Status of Massive Stars at the central parsec of the Milky Way
• Slow convection and fast rotation in crystallization-driven white dwarf dynamos
• Relative Importance of Convective Uncertainties
• 2M17091769+3127589: a mass-transfer binary with an extreme mass ratio
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
• Exploratory scenarios for the differential nuclear and tidal evolution of TZ Fornacis
• Planets Across Space and Time (PAST). II: Catalog and Analyses of the LAMOST-Gaia-Kepler Stellar Kinematic Properties
• KIC 3868420: A high-amplitude $\delta$ Scuti-$\gamma$ Dor hybrid star crossing the Hertzsprung gap
• Constraints on the Spindown of Fully-Convective M Dwarfs Using Wide Field Binaries
• A Synthetic Population of Ultra-Luminous X-ray Sources: Optical-X-ray Correlation
• EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
• BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• An upgraded interpolator of the radial basis functions network for spectral calculation based on empirical stellar spectral library
• Discovery of 34 low-mass comoving systems using NOIRLab Source Catalog DR2
• Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation
• Asteroseismology of the DAV star R808
• One's loss is (not) another's gain: Isotropic re-emission destabilizes mass transfer from radiative donor stars
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• Axion Instability Supernovae
• Detection horizon for the neutrino burst from the stellar helium flash
• Stellar multiplicity and stellar rotation: Insights from APOGEE
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• The Effect of Magnetization on Electron Heating in Low-Density Ultracold Neutral Plasmas
• Comprehensive analysis of a symbiotic candidate V503 Her
• Constraints on the Axion-Photon Coupling Using Stellar Modelling
• Excitation and Damping of Oscillation Modes in Gaseous Planets
• Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
• Massive star evolution revealed in the Mass-Luminosity plane
• Magnetic dynamos in white dwarfs -III: explaining the occurrence of strong magnetic fields in close double white dwarfs
• NGC 2004 #115: a black hole imposter containing three luminous stars
• K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant
• On the diversity of mixing and helium core masses of B-type dwarfs from gravity-mode asteroseismology
• Are There Pre-Main-Sequence/Black Hole X-ray Binaries?
• Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
• Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities
• Observational imprints of tidal internal gravity wave dissipation in star-planet systems