Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars

Abstract

We substantially update the capabilities of the open source software package Modules for Experiments in Stellar Astrophysics (MESA), and its one-dimensional stellar evolution module, MESA Star. Improvements in MESA Star's ability to model the evolution of giant planets now extends its applicability down to masses as low as one-tenth that of Jupiter. The dramatic improvement in asteroseismology enabled by the space-based Kepler and CoRoT missions motivates our full coupling of the ADIPLS adiabatic pulsation code with MESA Star. This also motivates a numerical recasting of the Ledoux criterion that is more easily implemented when many nuclei are present at non-negligible abundances. This impacts the way in which MESA Star calculates semi-convective and thermohaline mixing. We exhibit the evolution of 3-8 Msun stars through the end of core He burning, the onset of He thermal pulses, and arrival on the white dwarf cooling sequence. We implement diffusion of angular momentum and chemical abundances that enable calculations of rotating-star models, which we compare thoroughly with earlier work. We introduce a new treatment of radiation-dominated envelopes that allows the uninterrupted evolution of massive stars to core collapse. This enables the generation of new sets of supernovae, long gamma-ray burst, and pair-instability progenitor models. We substantially modify the way in which MESA Star solves the fully coupled stellar structure and composition equations, and we show how this has improved MESA's performance scaling on multi-core processors. Updates to the modules for equation of state, opacity, nuclear reaction rates, and atmospheric boundary conditions are also provided. We describe the MESA Software Development Kit (SDK) that packages all the required components needed to form a unified and maintained build environment for MESA. [Abridged]

Accepted for publication in The ApJ Supplement Series. Extra informations required to reproduce the calculations in this paper are available at http://mesastar.org/results/mesa2

References in corpus (114)

• Modules for Experiments in Stellar Astrophysics (MESA)
• The Dartmouth Stellar Evolution Database
• Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
• Accurate masses and radii of normal stars: modern results and applications
• Low Temperature Opacities
• Kepler Mission Design, Realized Photometric Performance, and Early Science
• The Palomar Transient Factory: System Overview, Performance and First Results
• Pre-Supernova Evolution of Massive Single and Binary Stars
• The Progenitor Stars of Gamma-Ray Bursts
• Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
• On the radiative equilibrium of irradiated planetary atmospheres
• Fast core rotation in red-giant stars revealed by gravity-dominated mixed modes
• On the Luminosity of Young Jupiters
• Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate
• Line and Mean Opacities for Ultracool Dwarfs and Extrasolar Planets
• A fossil origin for the magnetic fields of A-stars and white dwarfs
• Updated Electron-Conduction Opacities: The Impact on Low-Mass Stellar Models
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• Core-Accretion Model Predicts Few Jovian-Mass Planets Orbiting Red Dwarfs
• Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: I. Isothermal, Nonrotating, Radially Driven Flow
• Type Ib/c supernovae in binary systems I. Evolution and properties of the progenitor stars
• Exoplanet Atmospheres
• The Victoria-Regina Stellar Models: Evolutionary Tracks and Isochrones for a Wide Range in Mass and Metallicity that Allow for Empirically Constrained Amounts of Convective Core Overshooting
• ADIPLS -- the Aarhus adiabatic oscillation package
• Influence of gravity waves on the internal rotation and Li abundance of solar-type stars
• The N2K Consortium. II. A Transiting Hot Saturn Around HD 149026 With a Large Dense Core
• A variationally computed line list for hot NH3
• Turbulent Convection in Stellar Interiors. I. Hydrodynamic Simulation
• Stellar Companions to Stars with Planets
• Correcting stellar oscillation frequencies for near-surface effects
• Thermohaline mixing: A physical mechanism governing the photospheric composition of low-mass giants
• Sub-surface convection zones in hot massive stars and their observable consequences
• The VLT-FLAMES Tarantula Survey I: Introduction and observational overview
• ASTEC -- the Aarhus STellar Evolution Code
• Stellar evolution with rotation XII: Pre-supernova models
• Science performance of Gaia, ESA's space-astrometry mission
• On magnetic instabilities and dynamo action in stellar radiation zones
• Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014
• Evolution of massive stars with pulsation-driven superwinds during the RSG phase
• KOI-126: A Triply-Eclipsing Hierarchical Triple with Two Low-Mass Stars
• The evolution of runaway stellar collision products
• A Porosity-Length Formalism for Photon-Tiring-Limited Mass Loss from Stars Above the Eddington Limit
• Atmosphere, Interior, and Evolution of the Metal-Rich Transiting Planet HD 149026b
• The VLT-FLAMES survey of massive stars: Surface chemical compositions of B-type stars in the Magellanic Clouds
• Angular momentum transport in stellar interiors constrained by rotational splittings of mixed modes in red giants
• A uniform asteroseismic analysis of 22 solar-type stars observed by Kepler
• Asteroseismology of the solar analogs 16 Cyg A & B from Kepler observations
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• Forward seismic modelling of the pulsating magnetic B-type star HD 43317
• Tidal Dissipation and Obliquity Evolution in Hot Jupiter Systems
• Quasi-periodic eruptions from mildly eccentric unstable mass transfer in galactic nuclei
• Massive donors in interacting binaries: effect of metallicity
• Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
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• On the proper use of the Schwarzschild and Ledoux criteria in stellar evolution computations
• 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
• Structural glitches near the cores of red giants revealed by oscillations in g-mode period spacings from stellar models
• The i-process yields of rapidly-accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parameterizations from 3D hydrodynamics simulations
• The metallicity dependence of envelope inflation in massive stars
• Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars
• The dependence of convective core overshooting on stellar mass: reality check, and additional evidence
• Population III Binary Black Holes: Effects of Convective Overshooting on Formation of GW190521
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• The Warm Neptune GJ 3470b has a Polar Orbit
• Episodic mass ejections from common-envelope objects
• Asteroseismic signatures of evolving internal stellar magnetic fields
• Standing on the shoulders of giants: New mass and distance estimates for Betelgeuse through combined evolutionary, asteroseismic, and hydrodynamical simulations with MESA
• An extended halo around an ancient dwarf galaxy
• Orbital evolution of mass-transferring eccentric binary systems. II. Secular Evolution
• Tidally-Induced Radius Inflation of Sub-Neptunes
• Spoon-Feeding Giant Stars to Supermassive Black Holes: Episodic Mass Transfer from Evolving Stars and Their Contribution to the Quiescent Activity of Galactic Nuclei
• Helium abundance in a sample of cool stars: measurements from asteroseismology
• TESS Hunt for Young and Maturing Exoplanets (THYME) VI: an 11 Myr giant planet transiting a very low-mass star in Lower Centaurus Crux
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• Viscoelastic Tidal Dissipation in Giant Planets and Formation of Hot Jupiters Through High-Eccentricity Migration
• Disk Winds as an Explanation for Slowly Evolving Temperatures in Tidal Disruption Events
• WASP-4b Arrived Early for the TESS Mission
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• Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
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• Testing exoplanet evaporation with multi-transiting systems
• Inferences about supernova physics from gravitational-wave measurements: GW151226 spin misalignment as an indicator of strong black-hole natal kicks
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• Envelope Convection, Surface Magnetism and Spots in A- and late B-type Stars
• Common envelopes in massive stars: Towards the role of radiation pressure and recombination energy in ejecting red supergiant envelopes
• Evolution of Cataclysmic Variables and Related Binaries Containing a White-Dwarf
• On the photometric and spectroscopic diversity of Type II supernovae
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• KIC 10526294: a slowly rotating B star with rotationally split, quasi-equally spaced gravity modes
• Testing the radius scaling relation with $Gaia$ DR2 in the $Kepler$ field
• Spin-orbit alignment of exoplanet systems: ensemble analysis using asteroseismology
• The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component
• Long-term evolution of a magnetic massive merger product
• The K2-HERMES Survey: Age and Metallicity of the Thick Disc
• 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
• Effects of close binary evolution on the main-sequence morphology of young star clusters
• The surface nitrogen abundance of a massive star in relation to its oscillations, rotation, and magnetic field
• Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi
• The Contour Method: a new approach to finding modes of non-adiabatic stellar pulsations
• Chemically Homogeneous Evolution: A rapid population synthesis approach
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum II. Test of a revised prescription for transport by the Tayler instability
• Explaining iPTF14hls as a common envelope jets supernova
• On the Numerical Treatment and Dependence of Thermohaline Mixing in Red Giants
• Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3
• The spins of compact objects born from helium stars in binary systems
• Evolutionary tracks for Betelgeuse
• Evolution of Gas Giant Entropy During Formation by Runaway Accretion
• Shock Cooling Emission from Extended Material Revisited
• Chemical Abundances of Main-Sequence, Turn-off, Subgiant and red giant Stars from APOGEE spectra I: Signatures of Diffusion in the Open Cluster M67
• Radii and Mass-loss Rates of Type IIb Supernova Progenitors
• The Gaia-ESO Survey: open clusters in Gaia-DR1 - a way forward to stellar age calibration
• Recovering the star formation histories of recently-quenched galaxies: the impact of model and prior choices
• Heating of the Intergalactic Medium by Hydrogen Reionization
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• Metallicity-Dependent Signatures in the Kepler Planets
• Rotation of the convective core in $\gamma$ Dor stars measured by dips in period spacings of g modes coupled with inertial modes
• Numerical Simulations of Convective 3-Dimensional Red Supergiant Envelopes
• A stripped-companion origin for Be stars: clues from the putative black holes HR 6819 and LB-1
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• The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching and magnetic braking
• SN 2009ib: A Type II-P Supernova with an Unusually Long Plateau
• Quasi-periodic Eruptions from Helium Envelope of Hydrogen-deficient Stars Stripped by Supermassive Black Holes
• Hydrodynamic Simulations of the Interaction between an AGB Star and a Main Sequence Companion in Eccentric Orbits
• The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
• Triggering jet-driven explosions of core-collapse supernovae by accretion from convective regions
• Coping with loss: Stability of mass transfer from post-main sequence donor stars
• SN 2017ein and the Possible First Identification of a Type Ic Supernova Progenitor
• 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
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• On Carbon Burning in Super Asymptotic Giant Branch Stars
• Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity
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• Orbital evolution of mass-transferring eccentric binary systems. I. Phase-dependent evolution
• From Hot Jupiters to Super-Earths via Roche Lobe Overflow
• Discovery of ubiquitous lithium production in low-mass stars
• On the Diversity of Fallback Rates from Tidal Disruption Events with Accurate Stellar Structure
• APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
• The first ultracompact Roche lobe-filling hot subdwarf binary
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• Multi-Dimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin-Helium-Shell White Dwarfs
• Kepler-93b: A Terrestrial World Measured to within 120 km, and a Test Case for a New Spitzer Observing Mode
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• The spin rate of pre-collapse stellar cores: wave-driven angular momentum transport in massive stars
• The Ages of A-Stars I: Interferometric Observations and Age Estimates for Stars in the Ursa Major Moving Group
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• The orbits of subdwarf-B + main-sequence binaries: III. The period - eccentricity distribution
• 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
• Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution
• Common-envelope evolution with an asymptotic giant branch star
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• Low Mass X-ray Binaries: The Effects of the Magnetic Braking Prescription
• A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor
• On the formation of PSR J1640+2224: a neutron star born massive?
• The primordial and evolutionary abundance variations in globular-cluster stars: a problem with two unknowns
• Constructing stable 3D hydrodynamical models of giant stars
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• 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
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• Multi-Dimensional Radiative Transfer Calculations of Double Detonations of Sub-Chandrasekhar-Mass White Dwarfs
• Multi-Gigayear White Dwarf Cooling Delays from Clustering-Enhanced Gravitational Sedimentation
• The limited role of recombination energy in common envelope removal
• Multidimensional Simulations of Rotating Pair Instability Supernovae
• Tidal Dissipation in WASP-12
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• An Eccentric Massive Jupiter Orbiting a Sub-Giant on a 9.5 Day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images
• The Impact of Enhanced Iron Opacity on Massive Star Pulsations: Updated Instability Strips
• Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries and gravitational wave sources
• Bonn Optimized Stellar Tracks (BoOST). Simulated Populations of Massive and Very Massive Stars for Astrophysical Applications
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• Hybrid C-O-Ne white dwarfs as progenitors of type Ia supernovae: dependence on Urca process and mixing assumptions
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• Binary Asteroseismic Modelling: isochrone-cloud methodology and application to Kepler gravity-mode pulsators
• Wait for it: Post-supernova winds driven by delayed radioactive decays
• The surface abundances of Red Supergiants at core-collapse
• Constraining stellar evolution theory with asteroseismology of $\gamma$ Doradus stars using deep learning
• The formation of Cataclysmic Variables: the influence of nova eruptions
• The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
• Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance
• Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae
• Evaporation of dark matter from celestial bodies
• Probing the temperature gradient in the core boundary layer of stars with gravito-inertial modes: the case of KIC7760680
• Self-consistent predictions for LIER-like emission lines from post-AGB stars
• Modeling protoplanetary disk SEDs with artificial neural networks: Revisiting the viscous disk model and updated disk masses
• Bayesian Estimation of Thermonuclear Reaction Rates
• Analytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure
• Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7
• The BAyesian STellar Algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology
• Unicorns and Giraffes in the binary zoo: stripped giants with subgiant companions
• The Planetary Accretion Shock: I. Framework for Radiation-hydrodynamical Simulations and First Results
• Non-detection of Helium in the Upper Atmospheres of Three Sub-Neptune Exoplanets
• Structure and Evolution of Internally Heated Hot Jupiters
• 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
• 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
• Orbital Decay of Short-Period Exoplanets via Tidal Resonance Locking
• Triage of the Gaia DR3 astrometric orbits. I. A sample of binaries with probable compact companions
• Influence of Nuclear Reaction Rate Uncertainties on Neutron Star Properties Extracted From X-ray Burst Model-Observation Comparisons
• The age-metallicity dependence for white dwarfs
• Evolution of ONeMg Core in Super-AGB Stars towards Electron-Capture Supernovae: Effects of Updated Electron-Capture Rate
• Stellar and nebular diagnostics in the UV for star-forming galaxies
• Accretion onto Stars in the Disks of Active Galactic Nuclei
• Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow
• Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602
• The treatment of mixing in core helium burning models -- II. Constraints from cluster star counts
• Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy
• The Role of the Magnetorotational Instability in Massive Stars
• MESA meets MURaM: Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations
• Evolved Massive Stars at Low-metallicity V. Mass-Loss Rate of Red Supergiant Stars in the Small Magellanic Cloud
• Calibration of the Halpha Age-Activity relation for M dwarfs
• A Model for Fast Blue Optical Transient AT2018Cow: Circumstellar Interaction of a Pulsational Pair-instability Supernova
• The Planetary Accretion Shock. II. Grid of Post-Shock Entropies and Radiative Shock Efficiencies for Non-Equilibrium Radiation Transport
• The Close Binary Fraction as a Function of Stellar Parameters in APOGEE: A Strong Anti-Correlation With $\alpha$ Abundances
• Fingerprints of giant planets in the composition of solar twins
• A precise asteroseismic age and metallicity for HD 139614: a pre-main-sequence star with a protoplanetary disc in Upper-Centaurus Lupus
• Shock Breakout in 3-Dimensional Red Supergiant Envelopes
• Asteroseismic modelling of solar-type stars: internal systematics from input physics and surface correction methods
• Properties and Evolution of the Redback Millisecond Pulsar Binary PSR J2129-0429
• Revisiting nucleosynthesis in globular clusters: the case of NGC 2808 and the role of He and K
• On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars
• Formation of black holes in the pair-instability mass gap: evolution of a post-collision star
• 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
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• Carbon Shell or Core Ignitions in White Dwarfs Accreting from Helium Stars
• Tidal Inflation Reconciles Low-Density Sub-Saturns with Core Accretion
• Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity
• Properties of Carbon-Oxygen White Dwarfs From Monte Carlo Stellar Models
• Asteroseismic modeling of 16 Cyg A & B using the complete Kepler data set
• A New Model of Roche-lobe Overflow for Short-Period Gaseous Planets and Binary Stars
• Ultraviolet Detection of the Binary Companion to the Type IIb SN 2001ig
• Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen Poor Low Mass White Dwarf
• Testing asteroseismology with Gaia DR2: Hierarchical models of the Red Clump
• Consistent Modeling of GS 1826-24 X-ray Bursts for Multiple Accretion Rates Demonstrates the Possibility to Constrain rp-process Reaction Rates
• The Effect of Tides on the Population of PN from Interacting Binaries
• The Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phase
• The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
• The difficulty of inferring progenitor masses from Type II-Plateau supernova light curves
• White dwarf binaries suggest a common envelope efficiency $\alpha \sim 1/3$
• Triple system HD 201433 with a SPB star component seen by BRITE-Constellation: Pulsation, differential rotation, and angular momentum transfer
• Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars
• PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
• Rapid Rotation in the Kepler Field: Not a Single Star Phenomenon
• Kepler red-clump stars in the field and in open clusters: constraints on core mixing
• POET: A Model for (P)lanetary (O)rbital (E)volution due to (T)ides on Evolving Stars
• Angular momentum transport in massive stars and natal neutron star rotation rates
• Numerical Modeling of the Early Light Curves of Type IIP Supernovae
• Neutrinos from beta processes in a presupernova: probing the isotopic evolution of a massive star
• The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at $z=5.4$ with JWST/NIRCam in GOODS-S
• Modeling the early evolution of massive OB stars with an experimental wind routine
• The single-sided pulsator CO~Camelopardalis
• Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
• Suppression of quadrupole and octupole modes in red giants observed by Kepler
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• The Most Massive Heartbeat: An In-depth Analysis of ι Orionis
• Energy transport by convection in the common envelope evolution
• The Red-Giant Branch Bump Revisited: Constraints on Envelope Overshooting in a Wide Range of Masses and Metallicities
• Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars
• Opacity Driven Convection and Variability in Accretion Disks around Supermassive Black Holes
• A two-stage formalism for common-envelope phases of massive stars
• Stellar Rotation in the K2 Sample: Evidence for Modified Spindown
• Internal rotation of 13 low-mass low-luminosity red giants in the Kepler field
• Evolving LMXBs: CARB Magnetic Braking
• 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
• The Degree of Fine-Tuning in our Universe -- and Others
• Low-mass White Dwarfs with Hydrogen Envelopes as a Missing Link in the Tidal Disruption Menu
• Wolf-Rayet stars in the Small Magellanic Cloud as testbed for massive star evolution
• Hydrodynamical moving-mesh simulations of the tidal disruption of stars by supermassive black holes
• Low-frequency variability in massive stars: Core generation or surface phenomenon?
• Radiative-transfer models for explosions from rotating and non-rotating single WC stars. Implications for SN1998bw and LGRB/SNe
• Coupling thermal evolution of planets and hydrodynamic atmospheric escape in MESA
• i-Process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-Peak Neutron-Capture Elements
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• Statistical errors and systematic biases in the calibration of the convective core overshooting with eclipsing binaries. A case study: TZ Fornacis
• Pulsations of red supergiant pair-instability supernova progenitors leading to extreme mass loss
• Surface-effect corrections for oscillation frequencies of evolved stars
• Electron Capture Supernovae From Close Binary Systems
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• On the formation of eccentric millisecond pulsars with helium white-dwarf companions
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• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• KIC 4142768: An Evolved Gamma Doradus/Delta Scuti Hybrid Pulsating Eclipsing Binary with Tidally Excited Oscillations
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• Combined Effects of Rotation and Age Spreads on Extended Main Sequence Turn Offs
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• KIC 8164262: a Heartbeat Star Showing Tidally Induced Pulsations with Resonant Locking
• Spectroscopic Survey of γ Doradus Stars I. Comprehensive atmospheric parameters and abundance analysis of γ Doradus stars
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• Seismic measurement of the locations of the base of convection zone and helium ionization zone for stars in the {\it Kepler} seismic LEGACY sample
• Asteroseismic inference of the near-core magnetic field strength in the main sequence B star HD 43317
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• TOI-2109b: An Ultrahot Gas Giant on a 16 hr Orbit
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• WASP-4 is Accelerating Toward the Earth
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• Missing in Action: New Physics and the Black Hole Mass Gap
• Discovery of Extended Main Sequence Turn-offs in Four Young Massive Clusters in the Magellanic Clouds
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• Population synthesis of helium white dwarf--red giant star mergers and the formation of lithium-rich giants and carbon stars
• Light Curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers
• Constraints on explosive silicon burning in core-collapse supernovae from measured Ni/Fe ratios
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• An astrophysical interpretation of the remarkable g-mode frequency groups of the rapidly rotating $\gamma$ Dor star, KIC 5608334
• Extreme value statistics for two-dimensional convective penetration in a pre-Main Sequence star
• The Value of Progenitor Radius Measurements for Explosion Modeling of Type II-Plateau Supernovae
• Signatures of magnetic activity in the seismic data of solar-type stars observed by Kepler
• Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars
• Birth of the ELMs: a ZTF survey for evolved cataclysmic variables turning into extremely low-mass white dwarfs
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• How much hydrogen is in Type Ib and IIb supernova progenitors?
• Common envelope jets supernova (CEJSN) impostors resulting from a neutron star companion
• Benchmark ages for the Gaia benchmark stars
• Asteroseismology of luminous red giants with Kepler I: Long Period Variables with radial and non-radial modes
• Formation of sdB-stars via common envelope ejection by substellar companions
• The Physical Parameters of the Retired A Star HD185351
• Subdwarf B stars from the common envelope ejection channel
• Rossby and Magnetic Prandtl Number Scaling of Stellar Dynamos
• PSR J1012+5307: a millisecond pulsar with an extremely low-mass white dwarf companion
• A new class of pulsating hot subdwarfs
• Kepler Eclipsing Binaries with $\delta$ Scuti/$\gamma$ Doradus Pulsating Components 1: KIC 9851944
• Extended main-sequence turnoffs in the double cluster $h$ and $\chi$ Persei: The complex role of stellar rotation
• Stellar convective penetration: parameterized theory and dynamical simulations
• Very Massive Stars and Pair-Instability Supernovae: Mass-loss Framework for low Metallicity
• A Potential Progenitor for the Type Ic Supernova 2017ein
• Rotation in stellar interiors: General formulation and an asteroseismic-calibrated transport by the Tayler instability
• Ultra Long Gamma-Ray Bursts from the collapse of Blue Super Giant stars: an end-to-end simulation
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• Binarity and beyond in A stars I. Survey description and first results of VLTI/GRAVITY observations of VAST targets with high Gaia-Hipparcos accelerations
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• Planet Candidates from K2 Campaigns 5-8 and Follow-Up Optical Spectroscopy
• Excitation of gravity waves by fingering convection, and the formation of compositional staircases in stellar interiors
• Constraining the entropy of formation from young transiting planets
• The Importance of Urca-process Cooling in Accreting ONe White Dwarfs
• Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment
• Asteroseismology of 36 \emph{Kepler} subgiants -- I. Oscillation frequencies, linewidths and amplitudes
• Constraining differential rotation of Sun-like stars from asteroseismic and starspot rotation periods
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Population Synthesis of Black Hole X-Ray Binaries
• 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*
• Rejuvenated accretors have less bound envelopes: Impact of Roche lobe overflow on subsequent common envelope events
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• Convective Properties of Rotating Two-Dimensional Core-Collapse Supernova Progenitors
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• Photometric properties of reionization-epoch galaxies in the Simba simulations
• Angular momentum fluctuations in the convective helium shell of massive stars
• Planetary Engulfment in the Hertzsprung--Russell Diagram
• Measuring distances to low-luminosity galaxies using surface brightness fluctuations
• Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
• Ultra-compact X-ray binaries with He star companions
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• Radiative-transfer modeling of nebular-phase type II supernovae. Dependencies on progenitor and explosion properties
• The COMBS Survey -- II. Distinguishing the Metal-Poor Bulge from the Halo Interlopers
• Evolution of Wolf-Rayet stars as black hole progenitors
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• KIC 8262223: A Post-Mass Transfer Eclipsing Binary Consisting of a Delta Scuti Pulsator and a Helium White Dwarf Precursor
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• The Nearby Type Ibn Supernova 2015G: Signatures of Asymmetry and Progenitor Constraints
• The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
• Giant planet formation models with a self-consistent treatment of the heavy elements
• Pulsation-triggered dust production by asymptotic giant branch stars
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• Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
• Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• Faint rapid red transients from Neutron star -- CO white-dwarf mergers
• Semi-analytic Expressions for the Isolation and Coupling of Mixed Modes
• 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
• Coupled Thermal and Compositional Evolution of Photo Evaporating Planet Envelopes
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• A revisit of PSR J1909$-$3744 with 15-year high-precision timing
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• Radiating the hydrogen recombination energy during common envelope evolution
• Stochastic Low Frequency Variability in 3-Dimensional Radiation Hydrodynamical Models of Massive Star Envelopes
• Tidally Induced Pulsations in Kepler Eclipsing Binary KIC 3230227
• Evolutionary models for R Coronae Borealis stars
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• The Effects of Curvature and Expansion on Helium Detonations on White Dwarf Surfaces
• SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
• Binary Interaction Dominates Mass Ejection in Classical Novae
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• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
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• On the Origin of Sub-Subgiant Stars II: Binary Mass Transfer, Envelope Stripping, and Magnetic Activity
• A new hydrodynamics code for Type Ia Supernovae
• Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function
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• gyre_tides: Modeling binary tides within the gyre stellar oscillation code
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• Accretion-Induced Collapse From Helium Star + White Dwarf Binaries
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• TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full Frame Images
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• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
• Analysis of apsidal motion in eclipsing binaries using TESS data II. A test of internal stellar structure}
• Massive discs around low-mass stars
• SN 2020jfo: A short plateau Type II supernova from a low mass progenitor
• Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation
• Evolution models of helium white dwarf--main sequence star merger remnants
• 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
• Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition
• Lithium abundance and rotation of seismic solar analogues - Solar and stellar connection from Kepler and Hermes observations
• A $75\%$ Occurrence Rate of Debris Discs around F stars in the $\beta$ Pic Moving Group
• 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
• Hydrodynamical simulations and similarity relations for eruptive mass loss from massive stars
• On the nature of rapidly fading Type II supernovae
• Presupernova neutrinos: realistic emissivities from stellar evolution
• A prescription for the asteroseismic surface correction
• Star formation histories of the LEGUS dwarf galaxies (III): the non-bursty nature of 23 star forming dwarf galaxies
• Carbon-Oxygen Phase Separation in MESA White Dwarf Models
• On the Formation of Galactic Black Hole Low-Mass X-ray Binaries
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• TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars
• Transparent Helium in Stripped Envelope Supernovae
• Evolution of intermediate-mass X-ray binaries driven by magnetic braking of Ap/Bp stars: I. ultracompact X-ray binaries
• Tidal Circularization of Binaries by Resonance Locking I: The Importance of the Pre-Main-Sequence
• Seismic signature of electron degeneracy in the core of red giants: hints for mass transfer between close red-giant companions
• Multiple stellar populations along the red Horizontal Branch and Red Clump of Globular Clusters
• WDEC - A code for modeling white dwarf structure and pulsations
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• Search for surviving companions in type Ia supernova remnants
• Ejection of globular cluster interstellar media through ionization by white dwarfs
• RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich
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• Discovery of a double detonation thermonuclear supernova progenitor
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• The statistical challenge of constraining the low-mass IMF in Local Group dwarf galaxies
• Numerical experiments to help understand cause and effect in massive star evolution
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• Binarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC
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• Aluminium-26 from massive binary stars I: non-rotating models
• The role of radioactive nickel in shaping the plateau phase of Type II supernovae
• Modeling Supermassive Primordial Stars with MESA
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• The Dusty and Extremely Red Progenitor of the Type II Supernova 2023ixf in Messier 101
• Dynamical masses and mass-to-light ratios of resolved massive star clusters -- II. Results for 26 star clusters in the Magellanic Clouds
• Physical Properties of II Zw 40's Super Star Cluster and Nebula: New Insights and Puzzles from UV Spectroscopy
• Star formation in the first galaxies - III. Formation, evolution, and characteristics of the first stellar cluster
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• Red Supergiants in M31 and M33 I. The Complete Sample
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• Common envelopes in massive stars II: The distinct roles of hydrogen and helium recombination
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• A 3D radiation-hydrodynamic AGB binary model
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• The Primordial Entropy of Jupiter
• Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESA
• Dynamical tides in exoplanetary systems containing Hot Jupiters: confronting theory and observations
• Fundamental properties of Kepler and CoRoT targets: III. Tuning scaling relations using the first adiabatic exponent
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
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• The Aarhus red giants challenge II. Stellar oscillations in the red giant branch phase
• Numerical simulations of the random angular momentum in convection II: delayed explosions of red supergiants following "failed'' supernovae
• Radiation hydrodynamical simulations of eruptive mass Loss from progenitors of Type Ibn/IIn supernovae
• Mass loss of massive stars near the Eddington luminosity by core neutrino emission shortly before their explosion
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• On the Origin of Solar Torsional Oscillations and Extended Solar Cycle
• Testing White Dwarf Age Estimates using Wide Double White Dwarf Binaries from Gaia EDR3
• Post-common-envelope binary stars, radiative levitation, and blue large-amplitude pulsators
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• A comparative analysis of the observed white dwarf cooling sequence from globular clusters
• On The Development of Multidimensional Progenitor Models For Core-collapse Supernovae
• Shallower radius valley around low-mass hosts: Evidence for icy planets, collisions or high-energy radiation scatter
• Undetected Binary Stars Cause an Observed Mass Dependent Age Gradient in Upper Scorpius
• Pulsation in faint blue stars
• Accelerated Tidal Circularization Via Resonance Locking in KIC 8164262
• Explaining the differences in massive star models from various simulations
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• Type Ia Supernova Explosions from Hybrid Carbon-Oxygen-Neon White Dwarf Progenitors
• 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
• Physics and evolution of the most massive stars in 30 Dor. Mass loss, envelope inflation, and a variable upper stellar mass limit
• A seismic scaling relation for stellar age
• Asteroseismic modeling of gravity modes in slowly rotating A/F stars with radiative levitation
• Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au
• Detailed chemical abundances of stars in the outskirts of the Tucana II ultra-faint dwarf galaxy
• Evolving R Coronae Borealis Stars with MESA
• High-precision asteroseismology in Slowly Pulsating B star: HD 50230
• MESA models with magnetic braking
• Hydrogen in hot subdwarfs formed by double helium white dwarf mergers
• What are the spectroscopic binaries with high mass functions near the Gaia DR3 main sequence?
• Wave-driven mass loss of stripped envelope massive stars: progenitor-dependence, mass ejection, and supernovae
• The cosmic carbon footprint of massive stars stripped in binary systems
• A Complete Census of Luminous Stellar Variability on Day to Decade Timescales
• Enhancement of Lithium in Red Clump Stars by the Additional Energy Loss Induced by New Physics
• The Period-Luminosity Relations of Red Supergiants in M33 and M31
• Asteroseismology of the multiple stellar populations in the Globular Cluster M4
• Asteroseismic Fingerprints of Stellar Mergers
• The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
• Helium settling in F stars: constraining turbulent mixing using observed helium glitch signature
• The initial physical conditions of Kepler-36 b & c
• Evidence for the preferential disruption of moderately massive stars by supermassive black holes
• Nonlinear dynamical tides in white dwarf binaries
• Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
• Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
• PSR J1755$-$2550: A young radio pulsar with a massive, compact companion
• The Betelgeuse Project: Constraints from Rotation
• Capture of stars into gaseous discs around massive black holes: Alignment, circularization and growth
• Hot Start Giant Planets Form With Radiative Interiors
• New mass-loss rates of B supergiants from global wind models
• Internal rotation and inclinations of slowly pulsating B stars: Evidence of interior angular momentum transport
• Filling the Black Hole Mass Gap: Avoiding Pair Instability in Massive Stars through Addition of Non-Nuclear Energy
• Critical angular velocity and anisotropic mass loss of rotating stars with radiation-driven winds
• Star Formation Histories of the LEGUS Dwarf Galaxies (I): recent History of NGC1705, NGC4449 and Holmberg II
• Mass ejection in failed supernovae: equation of state and neutrino loss dependence
• Fast Blue Optical Transients due to Circumstellar Interaction and the Mysterious Supernova SN 2018gep
• Stellar Parameter Determination from Photometry using Invertible Neural Networks
• Re-inflation of warm and hot Jupiters
• Wide post-common envelope binaries from Gaia: orbit validation and formation models
• Neutronization During Carbon Simmering In Type Ia Supernova Progenitors
• PSR J1641+3627F: a low-mass He white dwarf orbiting a possible high-mass neutron star in the globular cluster M13
• Supernovae from massive stars with extended tenuous envelopes
• Linking chromospheric activity and magnetic field properties for late-type dwarf stars
• KIC 7582608: A new Kepler roAp star with frequency variability
• Supplying angular momentum to the jittering jets explosion mechanism using inner convection layers
• Tidally perturbed pulsations in the pre-main sequence $\delta$ Scuti binary RS Cha
• The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift
• Some Stars are Totally Metal: A New Mechanism Driving Dust Across Star-Forming Clouds, and Consequences for Planets, Stars, and Galaxies
• Dynamically inflated wind models of classical Wolf-Rayet stars
• A relation between the radial velocity dispersion of young clusters and their age: Evidence for hardening as the formation scenario of massive close binaries
• 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
• Asteroseismic Signatures of Core Magnetism and Rotation in Hundreds of Low-Luminosity Red Giants
• Tess asteroseismology of the known planet host star ${\lambda }^2$ Fornacis
• Analysis of apsidal motion in eclipsing binaries using TESS data: I. A test of gravitational theories
• Isochrone-cloud fitting of the extended Main-Sequence Turn-Off of young clusters
• Gravitational waves from in-spirals of compact objects in binary common-envelope evolution
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• 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
• Stellar modelling of Spica, a high-mass spectroscopic binary with a beta Cep variable primary component
• The EBLM Project VI. The mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey
• LAMOST Time-Domain Survey: First Results of four $K$2 plates
• Eclipsing binaries in the open cluster Ruprecht 147. I: EPIC 219394517
• Formation of hot subdwarf B stars with neutron star components
• Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?
• Convection Destroys the Core/Mantle Structure in Hybrid C/O/Ne White Dwarfs
• WD 1202-024: The Shortest-Period Pre-Cataclysmic Variable
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• 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
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• The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution
• SPYGLASS. III. The Fornax-Horologium Association and its Traceback History within the Austral Complex
• Disc-binary interactions in depleted post-AGB binaries
• Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
• A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
• 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
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• Kepler Object of Interest Network II. Photodynamical modelling of Kepler-9 over 8 years of transit observations
• Five young $\delta$ Scuti stars in the Pleiades seen with Kepler/K2
• The Araucaria Project. Accurate stellar parameters and distance to evolved eclipsing binary ASAS J180057-2333.8 in Sagittarius Arm
• Main Sequence Evolution with Layered Semiconvection
• Constraining transport of angular momentum in stars: Combining asteroseismic observations of core helium burning stars and white dwarfs
• Planet Engulfment Signatures in Twin Stars
• A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
• Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771
• Properties of the radius valley around low mass stars: Predictions from the core-powered mass-loss mechanism
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• Progenitors of Type IIb Supernovae: II. Observable Properties
• Schwarzschild and Ledoux are equivalent on evolutionary timescales
• Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
• Chemical Mixing Induced by Internal Gravity Waves in Intermediate Mass Stars
• 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?
• Formation of ultra-massive carbon-oxygen white dwarfs from the merger of carbon-oxygen and helium white dwarf pairs
• Hydrodynamic Simulations of Pre-Supernova Outbursts in Red Supergiants: Asphericity and Mass Loss
• Improved Main Sequence Turnoff Ages of Young Open Clusters: Multicolor UBV Techniques & the Challenges of Rotation
• On the necessity of composition-dependent low-temperature opacity in metal-poor AGB stars
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• The Binding Energy Parameter for Common Envelope Evolution
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• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
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• TOI-3235 b: a transiting giant planet around an M4 dwarf star
• Long-Term Lithium Abundance Signatures following Planetary Engulfment
• First solar models with OPAS opacity tables
• Evolved Massive Stars at Low-metallicity III. A Source Catalog for the Large Magellanic Cloud
• Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
• Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs
• Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
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• Deep Learning Applied to the Asteroseismic Modeling of Stars with Coherent Oscillation Modes
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• New $\beta$ Cep pulsators discovered with K2 space photometry
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
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• Atomic diffusion and turbulent mixing in solar-like stars: Impact on the fundamental properties of FG-type stars
• Masses of White Dwarf Binary Companions to Type Ia Supernovae Measured from Runaway Velocities
• Shock breakouts from red supergiants: analytical and numerical predictions
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• Convectively Driven Three Dimensional Turbulence in Massive Star Envelopes: I. A 1D Implementation of Diffusive Radiative Transport
• Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all
• Weak shock propagation with accretion. I. Self-similar solutions and application to failed supernovae
• Finding the First Cosmic Explosions. IV. 90 - 140 M${}_{\odot }$ Pair-Instability Supernovae
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
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• Radial Velocity Discovery of an Eccentric Jovian World Orbiting at 18 au
• Evolved Massive Stars at Low-metallicity II. Red Supergiant Stars in the Small Magellanic Cloud
• High-Energy X-ray Imaging of the Pulsar Wind Nebula MSH~15-52: Constraints on Particle Acceleration and Transport
• Predictions for gravity-mode periods and surface abundances in intermediate-mass dwarfs from shear mixing and radiative levitation
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Helium Enhanced Planets Along the Upper Edge of the Radius Valley
• A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
• Another Shipment of Six Short-Period Giant Planets from TESS
• Asteroseismic test of rotational mixing in low-mass white dwarfs
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• Towards a new era in giant exoplanet characterisation
• Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A
• Asymmetric core collapse of rapidly rotating massive star
• Planets on the Edge
• Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants
• Asteroseismic g-mode period spacings in strongly magnetic rotating stars
• Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods
• Novae heat their food: mass transfer by irradiation
• Detecting Pair-Instability Supernovae at z<5 with the James Webb Space Telescope
• Nonlinear regimes in mean-field full-sphere dynamo
• A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae
• The long-term evolution and appearance of Type Iax postgenitor stars
• Stellar Pulsations in Beyond Horndeski Gravity Theories
• Evolution and final fate of massive post-common-envelope binaries
• Magnetic activity evolution of solar-like stars: I. S_ph-Age relation derived from Kepler observations
• Period bouncers as detached magnetic cataclysmic variables
• 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
• Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernova
• Asteroseismic modelling of solar-type stars: A deeper look at the treatment of initial helium abundance
• LAMOST J0140355+392651: An evolved cataclysmic variable donor transitioning to become an extremely low mass white dwarf
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
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• HE 0430-2457: a post merger extremely low-mass pre-white dwarf in a wide binary posing as an extreme horizontal branch star
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• Electron Captures on ${}^{14}\mathrm{N}$ as a Trigger for Helium Shell Detonations
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• GRaM-X: A new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
• Velocity limits in the thermonuclear supernova ejection scenario for hypervelocity stars and the origin of US 708
• Thorough characterisation of the 16 Cygni system Part I: Forward seismic modelling with WhoSGlAd
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• Convective Mixing in Gas Giant Planets with Primordial Composition Gradients
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• The Loudest Stellar Heartbeat: Characterizing the most extreme amplitude heartbeat star system
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• The magneto-rotational instability in massive stars
• The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
• Hierarchically modelling Kepler dwarfs and subgiants to improve inference of stellar properties with asteroseismology
• Isochronal age-mass discrepancy of young stars: SCExAO/CHARIS integral field spectroscopy of the HIP 79124 triple system
• Explodability criteria for the neutrino-driven supernova mechanism
• Hot Electromagnetic Outflows. III. Displaced Fireball in a Strong Magnetic Field
• Effects of Irradiation on the Evolution of Ultra-compact X-ray Binaries
• Warm millimetre dust in protoplanetary discs near massive stars
• Magnetic braking with MESA evolutionary models in the single star and LMXB regimes
• On the energy source of ultra-stripped supernovae
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• Extreme isolation of WN3/O3 stars and implications for their evolutionary origin as the elusive stripped binaries
• SN 2022acko: the First Early Far-Ultraviolet Spectra of a Type IIP Supernova
• Forming merging double compact objects with stable mass transfer
• The IACOB project IX. Building a modern empirical database of Galactic O9-B9 supergiants: sample selection, description, and completeness
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• Planet-Induced Stellar Pulsations in HAT-P-2's Eccentric System
• Three long period transiting giant planets from TESS
• WOCS 5379: Detailed Analysis of the Evolution of a Post-Mass-Transfer Blue Straggler
• Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
• The Radius and Entropy of a Magnetized, Rotating Fully-convective Star: Analysis With Depth-dependent Mixing Length Theories
• A close-in giant planet escapes engulfment by its star
• Gaia-based Isochronal, Kinematic, and Spatial Analysis of the $\epsilon$ Cha Association
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• The effect of the centrifugal acceleration on period spacings of gravito-inertial modes in intermediate-mass stars
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• A possible formation channel for blue hook stars in globular cluster
• Magnetic field breakout from white dwarf crystallization dynamos
• Modeling overcontact binaries, I. The effect of tidal deformation
• WIYN Open Cluster Study. LXXXVII. HST Ultraviolet Detection of Hot White Dwarf Companions to Blue Lurkers in M67
• Investigating the Consistency of Stellar Evolution Models with Globular Cluster Observations via the Red Giant Branch Bump
• A red giant branch common envelope evolution scenario for the exoplanet WD 1856 b
• 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
• KIC 10736223: An Algol-type eclipsing binary just undergone the rapid mass-transfer stage
• Nature vs. Nurture: Distinguishing Effects from Stellar Processing and Chemical Evolution on Carbon and Nitrogen in Red Giant Stars
• X-Shooting ULLYSES: Massive Stars at low metallicity VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• Monte-Carlo methods for NLTE spectral synthesis of supernovae
• On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram
• GASTLI: An open-source coupled interior-atmosphere model to unveil gas giant composition
• Accounting for planet-shaped planetary nebulae
• Isochrone fitting of Galactic globular clusters - I. NGC 5904
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• Burst-induced coronal cooling in GS 1826-24 The clock wagging its tail
• A synthetic sample of short-cadence solar-like oscillators for TESS
• An accurate and efficient numerical calculation of detonation waves in multidimensional supernova simulations using a burning limiter and adaptive quasi-statistical equilibrium
• 3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
• An Analytical Density Profile of Dense Circumstellar Medium in Type II Supernovae
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• SPYGLASS. II. The Multi-Generational and Multi-Origin Star Formation History of Cepheus Far North
• On the existence of brown dwarfs more massive than the hydrogen burning limit
• Influence of a mass transfer stability criterion on double white dwarf populations
• Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters
• beta Cas: the first delta Scuti star with a dynamo magnetic field
• Modelling of Sigma Scorpii, a high-mass binary with a Beta Cep variable primary component
• Benchmarking MESA isochrones against the Hyades single star sequence
• Accreting CO material onto ONe white dwarfs towards accretion-induced collapse
• Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
• The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints
• The ASAS-SN Catalog of Variable Stars VIII: "Dipper" Stars in the Lupus Star-Forming Region
• Surface correction of main sequence solar-like oscillators with the $Kepler$ LEGACY sample
• Dynamical Masses and Stellar Evolutionary Model Predictions of M-Stars
• Precursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae
• Masses, Oxygen and Carbon abundances in CHEPS dwarf stars
• Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier?
• What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST
• Determining the seismic age of the young open cluster $\alpha$ Per using $\delta$ Scuti stars
• Asteroseismic Inference of Subgiant Evolutionary Parameters with Deep Learning
• The role of stellar expansion on the formation of gravitational wave sources
• Population of post-nova supersoft X-ray sources
• Energy Budget and Core-Envelope Motion in Common Envelope Evolution
• A Super-Eddington Wind Scenario for the Progenitors of Type Ia Supernovae
• The Asteroseismic Imprints of Mass Transfer: A Case Study of a Binary Mass Gainer in the SPB Instability Strip
• Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion
• A theory of mass transfer in binary stars
• Inverse Tides in Pulsating Binary Stars
• ASASSN-14dq: A fast-declining type II-P Supernova in a low-luminosity host galaxy
• 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
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• Contamination in TESS light curves: The case of the Fast Yellow Pulsating Supergiants
• Modeling contact binaries, II. The effect of energy transfer
• ArtPop: A Stellar Population and Image Simulation Python Package
• Sub-Chandrasekhar-mass detonations are in tension with the observed $t_0-M_{\text{Ni56}}$ relation of type Ia supernovae
• Limits on Mode Coherence in Pulsating DA White Dwarfs Due to a Non-static Convection Zone
• Theoretical tidal evolution constants for stellar models from the pre-main sequence to the white dwarf stage Apsidal motion constants, moment of inertia, and gravitational potential energy
• Revising Properties of Planet-Host Binary Systems. III. There is No Observed Radius Gap For Kepler Planets in Binary Star Systems
• Tidal migration of hot Jupiters: introducing the impact of gravity wave dissipation
• Core magnetic field imprint in the non-radial oscillations of red giant stars
• Modelling type IIP/IIL supernovae interacting with recent episodic mass ejections from their presupernova stars with MESA & SNEC
• Inferring the Rotation Period Distribution of Stars from their Projected Rotation Velocities and Radii: Application to late-F/early-G Kepler Stars
• A theoretical framework of BL Her stars. I. Effect of metallicity and convection parameters on period-luminosity and period-radius relations
• Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
• A Mass-accreting Gamma Doradus Pulsator with a Synchronized Core in Kepler Eclipsing Binary KIC 7385478
• 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
• TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• ZFOURGE: Extreme 5007$\mathring{A}$ emission may be a common early-lifetime phase for star-forming galaxies at $z>2.5$
• Mode identification in three pulsating hot subdwarfs observed with TESS satellite
• Low Mach Number Modeling of Convection in Helium Shells on Sub-Chandrasekhar White Dwarfs II: Bulk Properties of Simple Models
• TOI 694 b and TIC 220568520 b: Two Low-Mass Companions Near the Hydrogen Burning Mass Limit Orbiting Sun-like Stars
• Type Ia supernovae from non-accreting progenitors
• MOCMC: Method of Characteristics Moment Closure, a Numerical Method for Covariant Radiation Magnetohydrodynamics
• Formation of black widows through ultra-compact X-ray binaries with He star companions
• Super-Eddington winds from Type I X-ray bursts
• Asteroseismology of the ZZ Ceti star KUV 11370+4222
• The Art of Modeling Stellar Mergers and the Case of the B[e] Supergiant R4 in the Small Magellanic Cloud
• Photoionization Heating of Nova Ejecta by the Post-Outburst Supersoft Source
• 3D hydrodynamics simulations of internal gravity waves in red giant branch stars
• Is Thermohaline Mixing the Full Story? Evidence for Separate Mixing Events near the Red Giant Branch Bump
• Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators
• Isochrone fitting to the open cluster M67 in the era of Gaia and improved model physics
• A Short Intense Dynamo at the Onset of Crystallization in White Dwarfs
• Exploring the borderline between stable mass transfer and mergers in close binary evolution
• Searching for the Donor Stars of ULX Pulsars
• Confirming NGC 6231 as the parent cluster of the runaway high-mass X-ray binary HD 153919/4U 1700-37 with Gaia DR2
• The impact of pre-main sequence stellar evolution on midplane snowline locations and C/O in planet forming discs
• A nova re-accretion model for J-type carbon stars
• The Goldreich-Schubert-Fricke instability in stellar radiative zones
• Radio Emission from Supernovae in the Very Early Phase: Implications for the Dynamical Mass Loss of Massive Stars
• Evolution of Magnetized White Dwarf Binaries to Type Ia Supernovae
• ALMA reveals sunburn: CO dissociation around AGB stars in the globular cluster 47 Tucanae
• The Pulsation Properties of $\lambda$ Bootis Stars I. The Southern TESS Sample
• DSPS: Differentiable Stellar Population Synthesis
• The "Giraffe": Discovery of a stripped red giant in an interacting binary with a $\sim 2M_{\odot }$ lower giant
• The eclipsing binary systems with $\delta$ Scuti component. I. KIC 10661783
• X-Shooting ULLYSES: Massive Stars at low metallicity IX: Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud
• 3D Hydrodynamics of Pre-supernova Outbursts in Convective Red Supergiant Envelopes
• The K2 and TESS Synergy. I. Updated Ephemerides and Parameters for K2-114, K2-167, K2-237, and K2-261
• Radiative Acceleration of Dense Circumstellar Material in Interacting Supernovae
• From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
• The circularization timescales of late-type binary stars
• Testing stellar evolution with asteroseismic inversions of a main sequence star harboring a small convective core
• On the Launching and Structure of Radiatively Driven Winds in Wolf-Rayet Stars
• Aldebaran b's temperate past uncovered in planet search data
• Milky Way archaeology using RR Lyrae and type II Cepheids I. The Orphan stream in 7D using RR Lyrae stars
• Modeling R Coronae Borealis Stars: Effects of He-Burning Shell Temperature and Metallicity
• Dark matter capture and annihilation in stars: Impact on the red giant branch tip
• Simulating the negative jet feedback mechanism in common envelope jets supernovae
• Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies
• Influence of magnetic activity on the determination of stellar parameters through asteroseismology
• Possible Signatures of Ejecta-Companion Interaction in iPTF 13bvn
• Convective Excitation and Damping of Solar-like Oscillations
• SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
• The Effects of Asymmetric Dark Matter on Stellar Evolution I: Spin-Dependent Scattering
• On the maximum stellar rotation to form a black hole without an accompanying luminous transient
• HIP 33609 b: An Eccentric Brown Dwarf Transiting a V=7.3 Rapidly Rotating B-Star
• Mass transfer and magnetic braking in Sco X-1
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• New Insights for High-precision Asteroseismology: Acoustic Radius of KIC 6225718
• Mode Mixing and Rotational Splittings: II. Reconciling Different Approaches to Mode Coupling
• Centrifugally Driven Mass Loss and Outbursts of Massive Stars
• Convection and Overshoot in models of gamma Doradus and delta Scuti stars
• The Effects of Magnetic Fields on the Dynamics of Radiation Pressure Dominated Massive Star Envelopes
• Fast and Luminous Transients from the Explosions of Long Lived Massive White Dwarf Merger Remnants
• Observing and modelling the young solar analogue EK Draconis: starspot distribution, elemental abundances, and evolutionary status
• Evolution of Low-Mass X-ray Binaries: the Effect of Donor Evaporation
• Signatures of magnetic activity: On the relation between stellar properties and p-mode frequency variations
• Formation and Evolution of Blue Stragglers in 47 Tucanae
• On Binary Channels to Anomalous Cepheids
• An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
• Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star
• A systematic study of super-Eddington layers in the envelopes of massive stars
• Hydrodynamics and survivability during post-main-sequence planetary engulfment
• Pulsating B stars in the Scorpius-Centaurus Association with TESS
• Asteroseismology of the Double-Mode High-Amplitude $\delta$ Scuti Star VX Hydrae
• Mixed Mode Asteroseismology of Red Giant Stars Through the Luminosity Bump
• Hypercritical Accretion for Black Hole High Spin in Cygnus X-1
• Filling the gap between synchronized and non-synchronized sdBs in short-period sdBV+dM binaries with TESS: TIC 137608661, a new system with a well defined rotational splitting
• Convection and rotation boosted prescription of magnetic braking: application to the formation of extremely low-mass white dwarfs
• Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections
• Mixed Modes and Asteroseismic Surface Effects: I. Analytic Treatment
• Fundamental properties of Kepler and CoRoT targets -- IV. Masses and radii from frequencies of minimum $\Delta \nu$ and their implications
• Population synthesis of accreting white dwarfs: Rates and evolutionary pathways of H and He novae
• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• Observational predictions for Thorne-Żytkow objects
• Forecasting Chemical Abundance Precision for Extragalactic Stellar Archaeology
• A Moving Mesh Hydrodynamic Solver for ChaNGa
• Absolute dimensions of the eccentric eclipsing binary V541 Cygni
• A Spectroscopic and Photometric Investigation of the Mercury-Manganese Star KIC 6128830
• Extreme evaporation of planets in hot thermally unstable protoplanetary discs: the case of FU Ori
• DY Pegasi: An SX Phoenicis Star in a Binary System with an Evolved Companion
• Sensitivity of ${}^{44}$Ti and ${}^{56}$Ni production in CCSN shock-driven nucleosynthesis to reaction rates
• Alfvén wave-driven wind from RGB and AGB stars
• Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters
• HST/STIS analysis of the first main sequence pulsar CU Vir
• Torsional Oscillations in Dynamo Models with Fluctuations and Potential for Helioseismic Predictions of the Solar Cycles
• Calibrating angular momentum transport in intermediate-mass stars from gravity-mode asteroseismology
• The influence of line opacity treatment in STELLA on supernova light curves
• Evidence of an age gradient along the line of sight in the nuclear stellar disc of the Milky Way
• Chemical Abundances Of Open Clusters From High-Resolution Infrared Spectra. I. NGC 6940
• Exploring the Carbon Simmering Phase: Reaction Rates, Mixing, and the Convective Urca Process
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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
• Constraining Type Iax Supernova Progenitor Systems with Stellar Population Aging
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• A Black Hole Kicked At Birth: MAXI J1305-704
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• The effect of circumstellar matter on the double-peaked type Ic supernovae and implications for LSQ14efd, iPTF15dtg and SN 2020bvc
• A Population of Neutron Star Ultraluminous X-ray Sources with A Helium Star Companion
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• Eruption of the Envelope of Massive Stars by Energy Injection with Finite Duration
• Age-dating the young open cluster UBC 1 with g-mode asteroseismology, gyrochronology, and isochrone fitting
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• Tidally Tilted Pulsations in HD 265435, a subdwarf B Star with a Close White Dwarf Companion
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. V. Efficiency of the transport on the red giant branch and in the red clump
• Torsional oscillations and observed rotational period variations in early-type stars
• On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres
• SN 2016gsd: An unusually luminous and linear type II supernova with high velocities
• Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems is Dependent on Stellar Separation
• Dusty, Self-obscured Transients from Stellar Coalescence
• The GALAH survey: Co-orbiting stars and chemical tagging
• A window into $\delta$ Sct stellar interiors: Understanding the eclipsing binary system TT Hor
• Formation Scenario of the Progenitor of iPTF13bvn Revisited
• Orbital decay in an accreting and eclipsing 13.7 minute orbital period binary with a luminous donor
• Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
• The two-dimensional internal rotation of KIC11145123
• Dissecting the microphysics behind the metallicity-dependence of massive stars radii
• Age distribution of exoplanet host stars: Chemical and Kinematics age proxies from GAIA DR3
• TIC 308396022: a $\delta$ Scuti--$\gamma$ Doradus hybrid with large-amplitude radial fundamental mode and regular g-mode period spacing
• A comprehensive study of young B stars in NGC 2264: I. Space photometry and asteroseismology
• A 9-Hr CV With One Outburst in 4 Years of Kepler Data
• SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction
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• An updated modular set of synthetic spectral energy distributions for young stellar objects
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• CHIPS: Complete History of Interaction-Powered Supernovae
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• The young massive star cluster Westerlund 2 observed with MUSE. I. First results on the cluster internal motion from stellar radial velocities
• Beating stellar systematic error floors using transit-based densities
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• R Coronae Borealis Star Evolution: Simulating 3D Merger Events to 1D Stellar Evolution Including Large Scale Nucleosynthesis
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• Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
• A revisited study of Cepheids in open clusters in the Gaia era
• Aluminium-26 from massive binary stars III. Binary stars up to core-collapse and their impact on the early Solar System
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• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
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• Magnetic field evolution for crystallization-driven dynamos in C/O white dwarfs
• Rotation at the Fully Convective Boundary: Insights from Wide WD + MS Binary Systems
• Fast and Slow Crystallization-driven Convection in White Dwarfs
• A seven-Earth-radius helium-burning star inside a 20.5-min detached binary
• Constraints on the Progenitor System of SN 2016gkg from a Comprehensive Statistical Analysis
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• On the feasibility of structure inversions for gravity-mode pulsators
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• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
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• Bridging the Gap between Intermediate and Massive Stars I: Validation of MESA against the State-of-the-Art Monash Stellar Evolution Program for a 2$M_{\odot }$ AGB Star
• Pulsational instability of pre-main-sequence models from accreting protostars II. Modelling echelle diagrams of $\delta$ Scuti stars without rotational splitting
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• Inflated Eccentric Migration of Evolving Gas-Giants I: Accelerated Formation and Destruction of Hot and Warm Jupiters
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Year, Highly Eccentric Orbit
• Asteroseismic Inference of the Central Structure in a Subgiant Star
• Stellar Evolution and Tidal Dissipation in REBOUNDx
• Discovery of 18 stars with -3.10 < [Fe/H] < -1.45 in the Sagittarius dwarf galaxy
• Stellar populations and physical properties of starbursts in the Antennae galaxy from self-consistent modelling of MUSE spectra
• The Tayler Instability in the Anelastic Approximation
• Star Cluster Ages in the Gaia Era
• The impact of convective criteria on the properties of massive stars
• Asteroseismic inversions for radial differential rotation of Sun-like stars: ensemble fits
• Post-merger evolution of double helium white dwarfs and distribution of helium-rich hot subdwarfs
• Progenitor mass constraints for the type Ib intermediate-luminosity SN 2015ap and the highly extinguished SN 2016bau
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• Weak Shock Propagation with Accretion. II. Stability of Self-similar Solutions to Radial Perturbations
• Benchmarking Substellar Evolutionary Models Using New Age Estimates for HD 4747 B and HD 19467 B
• The WAGGS project -- III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity
• ODIN: Improved Narrowband Ly$\alpha$ Emitter Selection Techniques for $z$ = 2.4, 3.1, and 4.5
• TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field star
• Formation of long-period post-common-envelope binaries II. Explaining the self-lensing binary KOI 3278
• Intermediate Luminosity Optical Transients (ILOTs) from merging giants
• Type IIP Supernova Progenitors and their explodability I: Convective Overshoot, Blue Loops and Surface Composition
• WOCS 4540: Detailed Analysis of a Very Long Orbital Period Blue Straggler
• Intermediate-Mass Stars Become Magnetic White Dwarfs
• Isochrone fitting of Galactic globular clusters -- II. NGC6205 (M13)
• An update on fine-tunings in the triple-alpha process
• An efficient tidal dissipation mechanism via stellar magnetic fields
• Asteroseismic masses of four evolved planet-hosting stars using SONG and TESS: resolving the retired A-star mass controversy
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• Repeating Partial Tidal Encounters of Sun-like Stars Leading to their Complete Disruption
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
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• The K2 M67 Study: Precise Mass for a Turnoff Star in the Old Open Cluster M67
• The formation of subdwarf A-type stars
• The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars
• When does the onset of multiple stellar populations in star clusters occur-III: No evidence of significant chemical variations in main-sequence stars of NGC 419
• The imprint of star formation on stellar pulsations
• Comparison between the first and second mass eruptions from progenitors of Type IIn supernovae
• The spins of stripped B stars support magnetic internal angular momentum transport
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• The RR Lyrae Delay-Time Distribution: A Novel Perspective on Models of Old Stellar Populations
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• Multi-campaign Asteroseismic Analysis of eight Solar-like pulsating stars observed by the K2 mission
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• Unraveling the evolution of hot Jupiter systems under the effect of tidal and magnetic interactions and mass loss
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• Pulsation Analysis of High-Amplitude $\delta$ Scuti Stars with TESS
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• Photometric Classifications of Evolved Massive Stars: Preparing for the Era of Webb and Roman with Machine Learning
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• Mutual Inclination of Ultra-Short-Period Planets with Time Varying Stellar J2-moment
• The Chemical Composition of Extreme-Velocity Stars
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• The Impacts of Neutron-Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison
• Radio Transients from Newborn Black Holes
• Unresolved Rossby and gravity modes in 214 A and F stars showing rotational modulation
• The Influence of Disk Composition on the Evolution of Stars in the Disks of Active Galactic Nuclei
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• Optical Appearance of Eccentric Tidal Disruption Events
• Revising Properties of Planet-host Binary Systems I.: Methods and Pilot Study
• Rotational Variation Allows for Narrow Age Spread in the Extended Main Sequence Turnoff of Massive Cluster NGC 1846
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• Heavy Dark Matter in White Dwarfs: Multiple-Scattering Capture and Thermalization
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
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• A statistical test on the reliability of the non-coevality of stars in binary systems
• Frequency identification and asteroseismic analysis of the red giant KIC 9145955: fundamental parameters and helium core size
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• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb
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• Modeling the Thermal Bulge of A Hot Jupiter with the Two-Stream Approximation
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• Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri
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• Optical and Near-Infrared Excesses are Correlated in T Tauri Stars
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• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• Novae: An Important Source of Lithium in the Galaxy
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• Impact of central mixing scheme and nuclear reaction network on the extent of convective cores
• Red supergiant stars in IC 1613 and metallicity-dependent mixing length in the evolutionary model
• Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
• Evolution models of helium white dwarf--main-sequence star merger remnants: the mass distribution of single low-mass white dwarfs
• A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
• Gamma-Ray Light Curves and Spectra of Classical Novae
• A novel analytic atmospheric $T(\tau )$ relation for stellar models
• Hot Jupiter engulfment by a red giant in 3D hydrodynamics
• Photometric Investigation of Contact Binary DY Cet Based on TESS Data
• Relevance of the small frequency separation for asteroseismic stellar age, mass, and radius. A statistical investigation for main-sequence low-mass stars
• Distribution and evolution of Li abundance in red clump stars can be explained by the internal gravity waves
• The Impact of Tidal Migration of Hot Jupiters on the Rotation of Sun-like Main-sequence Stars
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Mixing via Thermocompositional Convection in Hybrid C/O/Ne White Dwarfs
• Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars
• Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge
• Modified Gravity and the Flux-weighted Gravity-Luminosity Relationship of Blue Supergiant Stars
• Binary Evolution: Roche Lobe Overflow and Blue Stragglers
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• Carbon 12C/13C isotope ratio of alpha Aurigae revised
• Gaia DR2 giants in the Galactic dust -- II. Application of the reddening maps and models
• The impact of magnetic fields on momentum transport and saturation of shear-flow instability by stable modes
• Probing red-supergiant atmospheres and winds with early-time high-cadence high-resolution type II supernova spectra
• Effect of Rotation on Wave Mixing in Intermediate Mass Stars
• ELM of ELM-WD: An extremely low mass hot star discovered in LAMOST survey
• Modelling stars with Gaussian Process Regression: Augmenting Stellar Model Grid
• Progenitors of Long-Duration Gamma-ray Bursts
• Dynamical Tides in Eccentric Binaries Containing Massive Main-Sequence Stars: Analytical Expressions
• Physical properties of the eclipsing binary KIC 9851944 and analysis of its tidally-perturbed p- and g-mode pulsations
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• Semi-Analytical Expression of G-Mode Period Spacing: The Case of Brunt-Väisälä Frequency with Not a Jump But a Ramp
• The Frequency and Mass-Ratio Distribution of Binaries in Clusters I: Description of the method and application to M67
• Enhanced mass-loss rate evolution of stars with $\gtrsim 18M_{\odot }$ and missing optically-observed type II core-collapse supernovae
• SCExAO/CHARIS Direct Imaging of A Low-Mass Companion At A Saturn-Like Separation from an Accelerating Young A7 Star
• Revising Properties of Planet-host Binary Systems II: Apparent Near-Earth Analog Planets in Binaries Are Often Sub-Neptunes
• Crust Cooling Models are Insensitive to the Crust-Core Transition Pressure for Realistic Equations of State
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• Storing magnetic fields in pre-collapse cores of massive stars
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• Asteroseismic Inversions for Internal Sound Speed Profiles of Main-sequence Stars with Radiative Cores
• The structure of detonation waves in supernovae revisited
• The imprint of convection on Type I X-ray bursts: Pauses in photospheric radius expansion lightcurves
• The evolution of magnetic hot massive stars: Implementation of the quantitative influence of surface magnetic fields in modern models of stellar evolution
• The Secular Periodic Evolution of X-ray Quasi-periodic Eruptions Driven by Star-disc Collisions
• Resonant Mode Coupling in $\delta$ Scuti Stars
• What governs the spin distribution of very young < 1 Myr low mass stars
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• On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations
• The mass distribution of the first stars can be determined via the 21-cm signal
• Stellar age determination in the Mass-Luminosity Plane
• Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
• Moving and Reactive Boundary Conditions in Moving-Mesh Hydrodynamics
• Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity
• Orbital radius during the grazing envelope evolution
• Semi-Transparent Shear Turbulence in Hot Jupiter Atmospheres
• Investigation of near-contact semi-detached binary W UMi through observations and evolutionary models
• Low energy core collapse supernovae in the frame of the jittering jets explosion mechanism
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
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• A catalog of new slowly pulsating B-type stars
• Towards 21st Century Stellar Models: Star Clusters, Supercomputing, and Asteroseismology
• Microlensing at Cosmological Distances: Event Rate Predictions in the Warhol Arc of MACS 0416
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• Observational Signatures of Carbon-Oxygen White Dwarf Merger Remnants
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• The ESO UVES/FEROS Large Programs of TESS OB pulsators. II. On the physical origin of macroturbulence
• HALO7D III: Chemical Abundances of Milky Way Halo Stars from Medium Resolution Spectra
• Convective blueshift strengths for 242 evolved stars
• Measuring mass transfer of AM CVn binaries with a space-based gravitational wave detector
• Type IIP Supernova Progenitors II: Stellar Mass and Obscuration by the Dust in the Circumstellar Medium
• Pulsations of intermediate-mass stars on the asymptotic giant branch
• WD mass and orbital period relation of sdB + He WD binaries
• Validating Stellar Abundance Measurements from Multi-Resolution Spectroscopy
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• On the Formation of SS433
• Comprehensive spectroscopic and photometric study of pulsating eclipsing binary star AI Hya
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• Characterising the AGB bump and its potential to constrain mixing processes in stellar interiors
• Comprehensive Bayesian Modeling of Tidal Circularization in Open Cluster Binaries part I: M 35, NGC 6819, NGC 188
• Tidal synchronization trapping in stars and planets with convective envelopes
• Planet-star interactions with precise transit timing. IV. Probing the regime of dynamical tides for GK host stars
• Stellar population synthesis based modelling of the Milky Way using asteroseismology of dwarfs and subgiants from Kepler
• Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests
• Common envelope jets supernova with thermonuclear outburst progenitor for the enigmatic supernova remnant W49B
• TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet
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• Ellipsars: Ring-like explosions from flattened stars
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• The core degenerate scenario for the type Ia supernova SN 2020eyj
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• Zahn's Theory of Dynamical Tides and Its Application to Stars
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• Change in the Orbital Period of a Binary System Due to Dynamical Tides for Main-Sequence Stars
• Convective Mixing: The Formation Channel of Li-rich Giants
• The S stars' zone of avoidance in the Galactic center
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• Search for Stellar Flybys in the Sco-Cen OB Association with the Gaia DR2
• Magnetic Webs in Stellar Radiative Zones
• Precise determination of stellar parameters of the ZZ Ceti and DAZ white dwarf GD 133 through asteroseismology
• 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
• Period-Colour and Amplitude-Colour relations for OGLE-$\delta$ Scuti stars in the Galactic Bulge and LMC
• On the nature of the core of $\alpha$ Centauri A: the impact of the metallicity mixture
• Revealing the Fate of Exoplanet Systems: Asteroseismic Identification of Host Star in the Red Clump or Red Giant Branch
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
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• The C/N ratio from FUV spectroscopy as a constraint upon the past evolution of HS0218+3229
• Anomalous orbital expansion of low-mass X-ray binary 2A 1822-371: the existence of a circumbinary disk?
• Photometric properties and stellar parameters of the rapidly rotating magnetic early-B star HD 345439
• Age and convective core overshooting calibrations in CPD-54 810 binary system. Statistical investigation on the solution robustness
• Confronting double-detonation sub-Chandrasekhar models with the low-luminosity suppression of Type Ia supernovae
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• A List of 49 New Stellar Twins from the Kepler Catalog of Eclipsing Binary Stars
• Rapid expansion of red giant stars during core helium flash by waves propagation to the envelope and implications to exoplanets
• A Possible Mechanism for Driving Oscillations in Hot Giant Planets
• He-shell flashes on the surface of oxygen-neon white dwarfs
• Mixed-mode coupling in the Red Clump I. Standard single star models
• The pre-SN activity as a possible explanation of the peculiar properties of Type IIP Supernova 2009kf
• Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models
• Suggested magnetic braking prescription derived from field complexity fails to reproduce the cataclysmic variable orbital period gap
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• Exploring the convective core of the high-amplitude $\delta$ Scuti star TIC 120857354 with asteroseismology
• V1082-Sgr: A magnetic cataclysmic variable with a lobe-filling companion star
• Observational Properties of 155 $\beta$ Cephei pulsating variable stars
• Capture rate of weakly interacting massive particles (WIMPs) in binary star systems
• Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra
• The First High-Contrast Images of X-Ray Binaries: Detection of Candidate Companions in the $\gamma$ Cas Analog RX J1744.7$-$2713
• Effects of Bound Diprotons and Enhanced Nuclear Reaction Rates on Stellar Evolution
• Dark Kinetic Heating of Exoplanets and Brown Dwarfs
• Kepler Object of Interest Network III. Kepler-82f: A new non-transiting $21 M_\bigoplus$ planet from photodynamical modelling
• Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae
• Spatio-temporal non-localities in a solar-like mean-field dynamo
• Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
• KIC 12268220: A $\delta$ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System
• Hydrodynamic simulations of WD-WD mergers and the origin of RCB stars
• Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
• Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers
• Comments on "Numerical Stability of Detonations in White Dwarf Simulations"
• Dynamical Masses and Ages of Sirius-like Systems
• Pre-supernova outbursts by core magnetic activity
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• On the rapid orbital expansion in the compact low-mass X-ray binary 2A 1822$-$371
• Interior rotation modelling of the $\beta$ Cep pulsator HD 192575 including multiplet asymmetries
• Angular momentum fluxes caused by Lambda-effect and meridional circulation structure of the Sun
• Light Curves and Event Rates of Axion Instability Supernovae
• In search of gravity mode signatures in main sequence solar-type stars observed by Kepler
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• 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
• The effects of Thomson scattering and chemical mixing on early-time light curves of double peaked type IIb supernovae
• Asteroseismology of the pre-main-sequence $\delta$ Scuti pulsator IP Persei
• X-ray binaries in M51 I: catalog and statistics
• Astrophysical Parameter Inference on Accreting White Dwarf Binaries using Gravitational Waves
• Convective dynamos of black widow companions
• A revisit to the enigmatic variable star 21 Comae
• Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
• Local disc model in view of Gaia DR1 and RAVE data
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• The Small Separation A-Star Companion Population: First Results with CHARA/MIRC-X
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Photometric variability of blue straggler stars in M67 with TESS and K2
• Quantification of Incertitude in Black Box Simulation Codes
• The Heating and Pulsations of V386 Serpentis after its 2019 Dwarf Nova Outburst
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• Converged simulations of the nozzle shock in tidal disruption events
• The Red Supergiant Progenitor of the Type II Supernova 2024abfl
• Eccentric grazing envelope evolution towards type IIb supernova progenitors
• SN 2016iyc: A Type IIb supernova arising from a low-mass progenitor
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Heavy element contributions of rotating massive stars to Interstellar Medium
• Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant
• Simulating the outcome of binary neutron star merger in common envelope jets supernovae
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• TIC 5724661: A Long-Period Binary with a Pulsating sdB Star and $\delta$ Scuti Variable
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
• A rapidly fading star as a type II obscuring intermediate luminosity optical transient (ILOT) in a triple star system
• Spallation-altered accreted compositions for X-ray bursts: Impact on ignition conditions and burst ashes
• Kepler Bonus: Aperture Photometry Light Curves of EXBA Sources
• The evolutionary and asteroseismic imprints of mass accretion. The 10 M${}_{\odot }$ $\beta$ Cep case study
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material
• Local two-dimensional simulations of the ignition of a helium shell detonation on a white dwarf by an impacting stream
• The convective kissing instability in low-mass M-dwarf models: convective overshooting, semi-convection, luminosity functions, surface abundances and star cluster age dating
• HD 42477: coupled r modes, g modes and a p mode in an A0Vnne star
• Exoplanet Occurrence Rate with Age for FGK Stars in Kepler
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Asteroseismology: Looking for axions in the red supergiant star Alpha Ori
• The double helium-white dwarf channel for the formation of AM CVn binaries
• Magnetic Fields or Overstable Convective Modes in HR 7495: Exploring the Underlying Causes of the Spike in the 'Hump & Spike' Features
• Lazarus Stars: Numerical investigations of stellar evolution with star-lifting as a life extension strategy
• Silicon Isotopic Composition of Mainstream Presolar SiC Grains Revisited: The Impact of Nuclear Reaction Rate Uncertainties
• Deciphering the period spacing pattern in the oscillation spectrum of the SPB star KIC 7760680
• Pre-supernova Ultra-light Axion-like Particles
• Residual eccentricity of an Earth-like planet orbiting a red giant Sun
• Tidally distorted barytropes and their Roche limits, with application to WASP-12b
• Stellar rotation and its connection to the evolution of hydrogen-dominated atmospheres of exoplanets
• GYRE: A New Open-Source Stellar Oscillation Code
• On the behaviour of spin-orbit connection of exoplanets
• A mixed helium-oxygen shell in some core-collapse supernova progenitors
• Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
• Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur
• Axion spectra and the associated x-ray spectra of low-mass stars
• A Strange Star Scenario for the Formation of Eccentric Millisecond Pulsar PSR J1946+3417
• Sodium enhancement in evolved cataclysmic variables
• Nonlinear pulsations of stars with initial mass 3 M_\odot on the asymptotic giant branch
• Binary stellar evolution yields in galactic chemical evolution calculations
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
• Exploring the internal rotation of the extremely low-mass He-core white dwarf GD 278 with TESS asteroseismology
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• Surface effects in solar-like oscillators
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC
• Weak or strong: coupling of mixed oscillation modes on the red-giant branch
• Fundamental properties of stars from Kepler and Gaia data: parallax offset and revised scaling relations
• Hydrodynamical simulations of proton ingestion flashes in Type I X-ray Bursts
• PTFO 8-8695: Two Stars, Two Signals, No Planet
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• The coevolution of migrating planets and their pulsating stars through episodic resonance locking
• Impacts of the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ reaction rate on ${}^{56}\mathrm{Ni}$ nucleosynthesis in pair-instability supernovae
• Structure and evolution of a tidally heated star
• The efficiency of mixed modes for angular momentum transport
• Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores
• Discovery of resonating integration modes in triple-mode high-amplitude $\delta$ Scuti stars: A new evolutionary phase indicator
• Mass transfer of low-mass binaries and chemical anomalies among unevolved stars in globular clusters
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• Further constraints on Jupiter's primordial structure
• Asteroseismology of KIC 8263801:Is it a member of NGC 6866 and a red clump star?
• A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources
• Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215.82+111745.0: a model with $p$-mode pulsations consistent with the observations
• Constraining dark photon properties with Asteroseismology
• The impact of rotation on the stochastic excitation of stellar acoustic modes in solar-like pulsators
• Evolutionary and Observational Properties of Red Giant Acoustic Glitch Signatures
• Gravity modes on rapidly rotating accreting white dwarfs and their variation after dwarf novae
• The evolutionary status of chemically peculiar eclipsing binary star DV Boo
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• Younger age for the oldest magnetic white dwarfs
• Thermal-timescale accretion does not always yield critical rotation in mass gainers
• Galactic cartography with SkyMapper: I. Population sub-structure and the stellar number density of the inner halo
• The Initial Magnetic Field Distribution in AB Stars
• How Rotation Affects Masses and Ages of Classical Cepheids
• Formation of millisecond pulsar-helium star binaries
• Constraining Accreted Neutron Star Crust Shallow Heating with the Inferred Depth of Carbon Ignition in X-ray Superbursts
• The Environments around W Serpentis Systems: Independent Limits on System Masses and Extended Envelopes
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• Effect of irradiation on the spin of millisecond pulsars
• The Effect of Dark Matter on Stars at the Galactic Center: The Paradox of Youth Problem
• White dwarf eccentricity fluctuation and dissipation by AGB convection
• Absolute dimensions of the F-type eclipsing binary V2154 Cygni
• The rotational shear in pre-collapse cores of massive stars
• Absolute dimensions of the early F-type eclipsing binary V506 Ophiuchi
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Empirical Relations for the Sensitivities of Solar-like Oscillations to Magnetic Perturbations
• HATS-34b and HATS-46b: Re-characterisation Using TESS and Gaia
• On the effect of pulsar evaporation on the cooling of white dwarfs
• Core-collapse supernova from a possible progenitor star of 100 M${}_{\odot }$
• Nonlinear tidal excitation of super-harmonic gravity waves in main-sequence stars in binary and exoplanetary systems
• A Trio of Giant Planets Orbiting Evolved Star HD 184010
• Variable Blue Straggler Stars in Open Cluster NGC 6819 Observed in the Kepler 'Superstamp' Field
• A uvbyCaHbeta CCD Analysis of the Open Cluster Standard, M67,and its Relation to NGC 752
• Neutrinos and Asteroseismology of Stars over the Helium Flash
• Ultrashort-period WD binaries are not undergoing strong tidal heating
• Twenty-three New Heartbeat Star Systems Discovered Based on TESS Data
• Searching for Galactic Red Supergiants with Gaia RVS Spectra
• On the Geometry of the Near-Core Magnetic Field in Massive Stars
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Beyond the Nyquist frequency: Asteroseismic catalog of undersampled Kepler late subgiants and early red giants
• Off-centre convective zones in mass accreting stellar models
• Wave-Driven Mixing Enhanced by Rotation in Red Giant Branch Stars
• Seismic detection of core magnetic fields in red giants using the gravity offset
• Drawing the line between explosion and collapse in electron-capture supernovae -- I. Impact of conductive flame speeds and ignition conditions on the explosion mechanism
• Asteroseismology and Buoyancy Glitch Inversion with Fourier Spectra of Gravity Mode Period Spacings
• Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
• Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Solar models with protosolar accretion and turbulent mixing
• Seismology and diffusion of ultramassive white dwarf magnetic fields
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Three-component Phase Separation for Ultramassive White Dwarf Models
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
• The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars
• Binary Stars Approaching Supermassive Black Holes: Hydrodynamics of Stellar Collisions, Mass Fallback and Partial TDEs
• Narrow absorption lines from intervening material in supernovae. II. Galaxy properties
• Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology
• Planetary Dynamos in Evolving Cold Gas Giants
• Thorne-Żytkow Objects
• Radiative acceleration calculation methods and abundance anomalies in Am stars
• Testing the sources of the peculiar abundances in globular clusters
• An irradiated-Jupiter analogue hotter than the Sun
• Impact of Asymmetrical Mass Ejection from Proto-White Dwarfs on the Properties of Binary Millisecond Pulsars
• A Close-in Planet Orbiting Giant Star HD 167768
• Constraining Axions with ZTF J1901+1458
• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
• Analyses of Hydrogen-stripped core-collapse supernovae using MOSFiT and MESA based tools
• Beyond binarity in A stars II. Disentangling the four stars in the vicinity of the triple HIP 87813 within the quintuple system HJ2814
• Constraining the Rotation Profile in a Low-Luminosity Subgiant with a Surface Rotation Measurement
• The K2 Galactic Archaeology Program: Overview, target selection and survey properties
• Where to find over-massive brown dwarfs: new benchmark systems for binary evolution
• Rotationally and tidally distorted compact stars A theoretical approach to the gravity-darkening exponents for white dwarfs
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Kepler Binary Stars in NGC 6819 Open Cluster: KIC 5113146 and KIC 5111815
• On rare core collapse supernovae inside planetary nebulae
• Digital Infrastructure in Astrophysics
• A Search For Pulsations in the Optical Light Curve of the Nova ASASSN-17hx
• Evolution and period change in RR Lyr variables of the globular cluster M 3
• A model of the Mira-type star T UMi
• Accretion of Planetary Material onto Host Stars
• K2 Observations of 95 Vir: delta Scuti Pulsations in a Chromospherically Active Star
• Ocean g-modes on transient neutron stars
• Second-generation planet formation after tidal disruption from common envelope evolution
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054
• A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters
• Helium enrichment during classical nova outbursts
• Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
• Influence of irradiation-driven winds on the evolution of intermediate-mass black hole X-ray binaries
• 3D non-LTE Ca II line formation in metal-poor FGK stars. I. Abundance corrections, radial velocity corrections, and synthetic spectra
• Star Formation for Predictive Primordial Galaxy Formation
• The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars
• Probing the Axion-Nucleon Coupling with Supergiant Stars
• Magnetic dynamos powered by white dwarf superficial convection
• A Continuous Galactic Line Source of Axions: The Remarkable Case of 23Na
• Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
• The rate of period change in DAV stars
• Pre-Supernova (Anti)Neutrino Emission Due to Weak-Interaction Reactions with Hot Nuclei
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Chemical abundances and doppler imaging of the Ap Si/He-wk star HD 100357
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
• 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
• Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars
• Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
• KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern
• 3D Convective Urca Process in a Simmering White Dwarf
• Structure formation in O-type stars and Wolf-Rayet stars
• On the parallelization of stellar evolution codes
• Foam: A Python package for forward asteroseismic modelling of gravity modes
• Irradiation effect and binary radio pulsars with giant companions
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• An Alternative Formation Scenario for Uranium-rich Giants: Engulfing a Earth-like Planet
• Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
• The SDSS-HET Survey of Kepler Eclipsing Binaries. A Sample of Four Benchmark Binaries
• Onset of common envelope evolution during a core helium flash by rapid envelope expansion
• Extraction of Physical Parameters of RRab Variables using Neural Network based Interpolator
• Collision of Two Stellar Associations in the Nearby Gum Nebula
• An Analytic, Fully Relativistic Framework for Tidal Disruption Event Streams in Schwarzschild Geometry
• Stellar response after stripping as a model for common-envelope outcomes
• Evolution of a Long-Lived Deep-Seated Main-Sequence Magnetic Field During White Dwarf Cooling
• The response of a red supergiant to a common envelope jets supernova (CEJSN) impostor event
• Explosions of pulsating red supergiants: a natural pathway for the diversity of Type II-P/L supernovae
• Asteroseismic modelling of the Binary HD 176465
• Good things come to those who wait: Watching donor stars evolve towards a mass-transfer instability
• A stringent upper limit on Be star fractions produced by binary interaction
• Partial, zombie, and full tidal disruption of stars by supermassive black holes
• Light Axion Emission and the Formation of Merging Binary Black Holes
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Understanding the cosmic abundance of ${}^{22}$Na: lifetime measurements in ${}^{23}$Mg
• Asteroseismology of low-mass stars: the balance between partial ionisation and Coulomb interactions
• Merged white dwarfs and nucleosynthesis
• Asteroseismology of sz lyn using multi-band high time resolution photometry from ground and space
• ${\tau }^9$ 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
• Study of the effects of magnetic braking on the lithium abundances of the Sun and solar-type stars
• The detached, evolved post-mass-exchange binary V643 Orionis
• Formation of massive close binaries I. Detached evolution
• The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations
• 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
• Discovery of a Highly Eccentric, Chromospherically Active Binary: ASASSN-V J192114.84+624950.8
• The depletion of the red supergiant envelope radiative zone during common envelope evolution
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
• Impact of Simultaneous Stellar Modeling Uncertainties on the Tip of the Red Giant Branch for Axion-Election Coupling
• Magellanic System Stars Identified in SMACS J0723.3-7327 James Webb Space Telescope Early Release Observations Images
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation
• 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
• Chemically peculiar stars on the pre-main sequence
• Discovery of Galactic center ejected star in DESI DR1
• Explanations for the two-component spectral energy distributions of gravitationally lensed stars at high redshifts
• Type Ia Supernovae from First-generation Stars
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• The Energy Sharing Timescale in an Analytic Framework for Common Envelope Hydrodynamics
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Jet-driven active galactic nucleus feedback in galaxy formation before black hole formation
• Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729
• Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects
• A 3D model for the stellar populations in the nuclei of NGC 1433,NGC 1566, and NGC 1808
• Near-critical magnetic fields in Kepler red giants
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• Icy Volatile Enhancements in Evolving Protoplanetary Disks
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri
• A new sample of massive B-type contact binary candidates from the OGLE survey of the Magellanic Clouds
• High-resolution spectroscopy of detached eclipsing binaries during total eclipses
• A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
• Blue Loops, Cepheids, and Forays into Axions
• VLTI observations of the Orion Belt stars: I. eps Orionis
• Advancing Globular Cluster Constraints on the Axion-Photon Coupling
• Evolved eclipsing binary systems in the Galactic bulge: Precise physical and orbital parameters of OGLE-BLG-ECL-305487 and OGLE-BLG-ECL-116218
• A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations
• Dynamical Mass Loss at the End of TP-AGB stars
• The influence of rotation and metallicity on the explodability of massive stars
• Can circumstellar interaction explain the strange light curve features of Type Ib/c supernovae?
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• Rare events of a peculiar thermonuclear supernova that precedes a core collapse supernova
• Analysis of TESS field eclipsing binary star V948 Her: a pulsating or non-pulsating star?
• Exploring the Small-scale Magnetic Fields in the Atmosphere of HD 49385 by Asteroseismic Analysis
• Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
• TULIPS: a Tool for Understanding the Lives, Interiors, and Physics of Stars
• A Lagrangian construction of rotating stars
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
• Asteroseismology of Massive Stars : Some Words of Caution
• A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
• 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
• Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars
• Exploring the physical properties of the $\gamma$ Dor binary star RX Dra with photometry and asteroseismology
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
• Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission
• Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars
• Using the Modified Lognormal Power Law Distribution to Model the Mass Function of NGC 1711
• Measuring Dust Masses of Protoplanetary Disks in Serpens and L1641/L1647 with ALMA
• 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
• Magneto-Archeology of White Dwarfs. Revisiting the fossil field scenario with observational constraints during the red giant branch
• 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
• Two unseen massive white dwarf candidates in close binaries
• Probing high-mass stellar evolutionary models with binary stars
• Ancient, eclipsing, tidally-locked: A blue lurker progenitor in the population of extreme-velocity star candidates
• Insights from Asteroseismology of Massive Stars: The Need for Additional Angular Momentum Transport Mechanisms
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Asteroseismic Constraints on the Models of Hot B Subdwarfs: Convective Helium-Burning Cores
• Probing Thin Winds in Massive OB Stars of the SMC with JWST/NIRSPEC Br-alpha Spectroscopy
• On the emergence of a new instability during core-collapse of very massive stars
• The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
• Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
• NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists
• Double-faced white dwarfs and the magnetic inhibition of convection
• Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
• CY Aquarii: A Triple System with Twin Companions
• Critical Metallicity of Cool Supergiant Formation. II. Physical Origin
• Chameleon Mechanism in Inhomogeneous Astrophysical Objects
• The Thermal Pulses of Very-Low-Mass Stars
• Evolution and Explosion of Massive Stars Leading to IIP-IIL SNe with MESA and SNEC
• On the nature of the candidate T-Tauri star V501 Aurigae
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts
• On the non-dissipative orbital evolution of a binary system comprising non-compact components with misaligned spin and orbital angular momenta
• Neutrinos from stars in the Milky Way
• Patchy nightside clouds on ultra-hot Jupiters: General Circulation Model simulations with radiatively active cloud tracers
• Accretion induced merger leading to core collapse supernovae in old stellar populations
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• Sub-photospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves
• Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
• Discovery of a runaway star likely ejected by a Type Iax Supernova
• Are There Pre-Main-Sequence/Black Hole X-ray Binaries?
• Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies
• Absolute physical parameters of three poorly studied detached eclipsing binaries
• Detailed Characterization of Heartbeat Stars and their Tidally Excited Oscillations
• Validation of the Gaia Early Data Release 3 parallax zero-point model with asteroseismology
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Radio observations of massive stars in the Galactic centre: The Quintuplet cluster
• Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events
• Stellar multiplicity and stellar rotation: Insights from APOGEE
• Faint intermediate luminosity optical transients (ILOTs) from engulfing exoplanets on the Hertzsprung gap
• Inflated Eccentric Migration of evolving gas giants II: Numerical methodology and basic concepts
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution
• K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant
• Stationary accretion flow with nuclear burning
• Discovery of 34 low-mass comoving systems using NOIRLab Source Catalog DR2
• Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities
• Primordial black holes capture by stars and induced collapse to low-mass stellar black holes
• A New Versatile Code for Gamma-Ray Monte-Carlo Radiative Transfer
• Magellan/IMACS spectroscopy of Grus I: A low metallicity ultra-faint dwarf galaxy
• Exploratory scenarios for the differential nuclear and tidal evolution of TZ Fornacis
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Asteroseismic Diagnostics for Semi-Convection in B Stars in the Era of K2
• Comprehensive analysis of a symbiotic candidate V503 Her
• Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation
• Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
• Three-dimensional simulations of accretion disks in pre-CE systems
• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
• Expectation for the MeV Gamma-Ray Emission from Pair-Instability Supernovae
• Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption
• A Black Hole is Born: 3D GRMHD Simulation of Black Hole Formation from Core-Collapse
• The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars
• The Cooling of Old White Dwarfs in 47 Tucanae
• Evolution of the ZTF SLRN-2020 star-planet merger
• Inactive longitude and superflare in the active single-lined pre-main sequence binary V2279 Cyg
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• Attempting an accurate age estimate of the open cluster NGC 6633 using CoRoT and Gaia
• Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope
• 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
• Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA
• Apsidal motion and proximity effects in the massive binary BD+60 497
• Physical interpretation of the oscillation spectrum on the RGB and AGB
• Ensemble seismic study of the properties of the core of Red Clump stars
• Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• Heavy dark matter in rapidly evolving massive stars
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• 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
• Detection horizon for the neutrino burst from the stellar helium flash
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• Excitation and Damping of Oscillation Modes in Gaseous Planets
• Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
• On the Importance of the Convective Urca Process in 3D Simulations of a Simmering White Dwarf
• Observational imprints of tidal internal gravity wave dissipation in star-planet systems
• Tidal capture and repeating partial tidal disruption events of giant stars
• 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
• Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
• Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid
• A Theoretical Study of the Structure and Elemental Abundances of HD 20794
• Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
• Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss
• Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
• 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
• Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
• 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
• The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• 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
• Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
• A Warm Massive Pair of Planets around TOI-1232 Revealed with Transit-timing Variations and Doppler Spectroscopy
• Formation of black holes from He stars
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
• One's loss is (not) another's gain: Isotropic re-emission destabilizes mass transfer from radiative donor stars
• Gravitational-Wave Signatures of Massive Black Hole Formation
• The reason for the occurrence of W-type contact binaries
• Detectability of compact intermediate-mass black hole binaries as low-frequency gravitational wave sources: the influence of dynamical friction of dark matter
• Can the Anomalous Magnetic Braking of Ap/Bp Stars Explain the Orbital Decay of Algol-type Binaries?
• The bimodal distribution of donor stars in X-ray binaries
• Discerning internal conditions of pulsating hot subdwarf B stars. Modelling multiple trapped modes in KIC 10001893
• Huntsman may need to be irradiated
• Eighteen Exoplanet Host Stars from the NPOI Data Archive
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• Constraints on the Axion-Photon Coupling Using Stellar Modelling
• MESA-Web: A cloud resource for stellar evolution in astronomy curricula
• HIP 67506 C: MagAO-X Confirmation of a New Low-Mass Stellar Companion to HIP 67506 A
• Constraints on the Spindown of Fully-Convective M Dwarfs Using Wide Field Binaries
• Potential Habitability as a Stellar Property: Effects of Model Uncertainties and Measurement Precision
• Atmospheric mass loss and stellar wind effects in young and old systems II: Is TOI-942 the past of TOI-421 system?
• NGC 2004 #115: a black hole imposter containing three luminous stars
• Slow convection and fast rotation in crystallization-driven white dwarf dynamos
• Axion Instability Supernovae
• On the diversity of mixing and helium core masses of B-type dwarfs from gravity-mode asteroseismology
• Possible in situ formation of Uranus and Neptune via Pebble Accretion
• Star formation in two irradiated globules around Cygnus OB2
• Convective Penetration in Early-Type Stars
• Viscous and centrifugal instabilities of massive stars
• A Multi-Planet System's Sole Super-Puff: Exploring Allowable Physical Parameters for the Cold Super-Puff HIP 41378 f
• Magnetic dynamos in white dwarfs -III: explaining the occurrence of strong magnetic fields in close double white dwarfs
• TYC~2990-127-1: an Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer
• Can small-scale magnetic fields be the major cause for the near-surface effect of the solar p-mode frequencies?
• StelNet: Hierarchical Neural Network for Automatic Inference in Stellar Characterization
• Pulsations of blue supergiants before and after helium core ignition
• Damping of Oscillations in Red Giants by Resonant Mode Coupling
• The COMBS Survey -- III. The Chemodynamical Origins of Metal-Poor Bulge Stars
• Planets Across Space and Time (PAST). II: Catalog and Analyses of the LAMOST-Gaia-Kepler Stellar Kinematic Properties
• 2M17091769+3127589: a mass-transfer binary with an extreme mass ratio
• Formation, diffusion and accreting pollution of DB white dwarfs
• Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
• 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
• OO Dra: an Algol-type binary formed through an extremely helium-poor mass accretion revealed by asteroseismology
• Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2
• PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators
• Urca Nuclide Production in Type-I X-ray Bursts and Implications for Nuclear Physics Studies
• An upgraded interpolator of the radial basis functions network for spectral calculation based on empirical stellar spectral library
• Relative Importance of Convective Uncertainties