Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions

Abstract

We update the capabilities of the software instrument Modules for Experiments in Stellar Astrophysics (MESA) and enhance its ease of use and availability. Our new approach to locating convective boundaries is consistent with the physics of convection, and yields reliable values of the convective core mass during both hydrogen and helium burning phases. Stars with $M<8{\mathrm{M}}_{\odot }$ become white dwarfs and cool to the point where the electrons are degenerate and the ions are strongly coupled, a realm now available to study with MESA due to improved treatments of element diffusion, latent heat release, and blending of equations of state. Studies of the final fates of massive stars are extended in MESA by our addition of an approximate Riemann solver that captures shocks and conserves energy to high accuracy during dynamic epochs. We also introduce a 1D capability for modeling the effects of Rayleigh-Taylor instabilities that, in combination with the coupling to a public version of the STELLA radiation transfer instrument, creates new avenues for exploring Type II supernovae properties. These capabilities are exhibited with exploratory models of pair-instability supernova, pulsational pair-instability supernova, and the formation of stellar mass black holes. The applicability of MESA is now widened by the capability of importing multi-dimensional hydrodynamic models into MESA. We close by introducing software modules for handling floating point exceptions and stellar model optimization, and four new software tools -- MESAWeb, MESA-Docker, pyMESA, and mesastar.org -- to enhance MESA's education and research impact.

arXiv comment64 pages, 61 figures; Accepted to AAS Journals

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• Internal Gravity Waves in Massive Stars II: Frequency Analysis Across Stellar Mass
• Common Envelope Wind Tunnel: Range of Applicability and Self-Similarity in Realistic Stellar Envelopes
• 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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• Systematic investigation of the effect of 56Ni mixing in the early photospheric velocity evolution of stripped-envelope supernovae
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• Stellar Evolution and Tidal Dissipation in REBOUNDx
• 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
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• Weak Shock Propagation with Accretion. II. Stability of Self-similar Solutions to Radial Perturbations
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• An Investigation of Non-Canonical Mixing in Red Giant Stars Using APOGEE 12C/13C Ratios Observed in Open Cluster Stars
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• Intermediate Luminosity Optical Transients (ILOTs) from merging giants
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• WOCS 4540: Detailed Analysis of a Very Long Orbital Period Blue Straggler
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• Unveiling the Nature of SN 2011fh: a Young and Massive Star Gives Rise to a Luminous SN 2009ip-like Event
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• On the orbital decay of the gas giant Kepler-1658b
• Exoplanet atmosphere evolution: emulation with neural networks
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• Exploring the convective core of the hybrid $\delta$ Scuti-$\gamma$ Doradus star CoRoT 100866999 with asteroseismology
• Three-Dimensional Simulations of Massive Stars: II. Age Dependence
• DES16C3cje: A low-luminosity, long-lived supernova
• Tidal evolution and diffusive growth during high-eccentricity planet migration: revisiting the eccentricity distribution of hot Jupiters
• Comprehensive UV and Optical spectral analysis of Cygnus X-1: Stellar and wind parameters, abundances, and evolutionary implications
• Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates
• The impact of composition choices on solar evolution: age, helio- and asteroseismology, and neutrinos
• Mirror principle and the red-giant bump: the battle of entropy in low-mass stars
• Stochastic excitation of internal gravity waves in rotating late F-type stars: A 3D simulation approach
• The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations
• A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
• Structural and Evolutionary Diagnostics from Asteroseismic Phase Functions
• TIC 290061484: A Triply Eclipsing Triple System with the Shortest Known Outer Period of 24.5 Days
• Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars
• Optimal Celestial Bodies for Dark Matter Detection
• The formation of type Ia supernovae from carbon-oxygen-silicon white dwarfs
• Modelling of the B-type binaries CW Cep and U Oph: A critical view on dynamical masses, core boundary mixing, and core mass
• Mixed Modes and Asteroseismic Surface Effects: II. Subgiant Systematics
• SN 1961V: A Pulsational Pair-Instability Supernova
• Formation and Evolution of Accreting Compact Objects
• The Wolf-Rayet Stellar Response To The Iron Opacity Bump: Envelope Inflation, Winds, and Microturbulence
• The Three-Dimensional Collapse of a Rapidly Rotating 16 $M_{\odot }$ Star
• Minimum Orbital Period of Pre-Cataclysmic Variables
• Orbital and physical parameters of eclipsing binaries from the ASAS catalogue -- XII. A sample of systems with $K2$ photometry
• Thermonuclear and Electron-Capture Supernovae from Stripped-Envelope Stars
• The Symbiotic X-ray Binary IGR J16194-2810: A Window on the Future Evolution of Wide Neutron Star Binaries From Gaia
• Connecting integrated RGB mass loss from asteroseismology and globular clusters
• Pulsational properties of ten new slowly pulsating B stars
• On the role of reduced wind mass-loss rate in enabling exoplanets to shape planetary nebulae
• Properties of the Hyades, the eclipsing binary HD27130, and the oscillating red giant $\epsilon$ Tau
• To be or not to be a black hole: detailed binary population models as a sanity check
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Regular Radial Velocity Variations in Nine G- and K-type Giant Stars: Eight Planets and One Planet Candidate
• The hydrogen clock to infer the upper stellar mass
• Modeling of multimode radially pulsating High-Amplitude Delta Scuti stars from the OGLE Galactic bulge sample
• Unraveling the evolution of hot Jupiter systems under the effect of tidal and magnetic interactions and mass loss
• Platform for Probing Radiation Transport Properties of Hydrogen at Conditions Found in the Deep Interiors of Red Dwarfs
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• Rotational modulation in A and F stars: Magnetic stellar spots or convective core rotation?
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey: III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-Transit Jupiter Orbiting TOI-2010
• Three Dimensional Natures of Massive Star Envelopes
• The effect of the adiabatic assumption on asteroseismic scaling relations for luminous red giants
• TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence
• An absolute mass, precise age, and hints of planetary winds for WASP-121 A and b from a JWST NIRSpec phase curve
• The bulk metallicity of giant planets around M stars
• The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars
• Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
• Can GW231123 have a stellar origin?
• The mass distribution of stars stripped in binaries: The effect of metallicity
• Empirical instability strip for classical Cepheids: I. The LMC galaxy
• Synthesizing Spectra from 3D Radiation Hydrodynamic Models of Massive Stars Using Monte Carlo Radiation Transport
• Effects of Winds on the Optical Properties of Type Ib and Ic Supernova Progenitors
• Tides in the high-eccentricity migration of hot Jupiters: Triggering diffusive growth by nonlinear mode interactions
• A rapidly evolving high-amplitude $\delta$ Scuti star crossing the Hertzsprung Gap
• The RR Lyrae Delay-Time Distribution: A Novel Perspective on Models of Old Stellar Populations
• Mass ratio, the hills mechanism, and the galactic centre S-stars
• Pulsation-driven mass loss from massive stars behind stellar mergers in metal-poor dense clusters
• Tidal Dissipation in Evolved Low and Intermediate Mass Stars
• EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope
• Li-rich and super Li-rich giants produced by element diffusion
• Detached and Continuous Circumstellar Matter in Type Ibc Supernovae from Mass Eruption
• The Evolution of Accreting Population III Stars at 10${}^{-6}$-10${}^3$ M${}_{\odot }$/yr
• Stellar Shocks From Dark Matter Asteroid Impacts
• Mode Mixing and Rotational Splittings: I. Near-Degeneracy Effects Revisited
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• SN 2018hna: Adding a Piece to the Puzzles of the Explosion of Blue Supergiants
• Convective overshooting in sdB stars using the $k$-$\omega$ model
• Pulsation Analysis of High-Amplitude $\delta$ Scuti Stars with TESS
• Mechanical feedback from black hole accretion as an energy source of core-collapse supernova explosions
• Unveiling complex magnetic field configurations in red giant stars
• A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
• Searching for the Next Galactic Luminous Red Nova
• Evolution of Main-Sequence-like Surviving Companions in Type Ia Supernova Remnants
• SN 2017czd: A Rapidly Evolving Supernova from a Weak Explosion of a Type IIb Supernova Progenitor
• Dynamical Screening Effects on Big Bang Nucleosynthesis
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• UOCS-IX. AstroSat/UVIT study of the open cluster NGC 2818: Blue Stragglers, Yellow Stragglers, Planetary Nebula, and their membership
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• Discrepant Approaches to Modeling Stellar Tides, and the Blurring of Pseudosynchronization
• An upper limit on the spins of merging binary black holes formed through binary evolution
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• The formation of the magnetic symbiotic star FN Sgr
• Constraining mass transfer and common-envelope physics with post-supernova companion monitoring
• Gaia BH1 and BH2 -- evolutionary models with overshooting of the black hole progenitors within the present-day binary separation
• Magnetic Field Evolution of Hot Exoplanets
• The SOPHIE search for northern extrasolar planets. XVIII: Six new cold Jupiters, including one of the most eccentric exoplanet orbits
• Frequency analysis of KIC 1573174 : shedding light on the nature of HADS stars
• Whispering in the dark: Faint X-ray emission from black holes with OB star companions
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• Lithium in red giants: the roles of the He-core flash and the luminosity bump
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• A discontinuity in the luminosity-mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap
• Precise Evolutionary Asteroseismology of High-Amplitude δ Scuti Star AE Ursae Majoris
• Origin and Evolution of Angular Momentum of Class II Disks
• Dynamical parallax, physical parameters and evolutionary status of the components of the bright eclipsing binary α Draconis
• Premature Black Hole Death of Population III Stars by Dark Matter
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• The Maximum Black Hole Mass at Solar Metallicity
• The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at $\approx$2 AU
• The Pre-main Sequence: Challenges and Prospects for Asteroseismology
• Quantifying How Density Gradients and Front Curvature Affect Carbon Detonation Strength During Type Ia Supernovae
• Nonlinear Mixed Modes in Red Giants
• Comparing Moment-Based and Monte Carlo Methods of Radiation Transport Modeling for Type II-Plateau Supernova Light Curves
• The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures
• Photometric White Dwarf Rotation
• Discovery, TESS Characterization, and Modeling of Pulsations in the Extremely Low Mass White Dwarf GD 278
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Asteroseismology of RRab variable star EZ Cnc from K2 photometry and LAMOST spectroscopy
• Transition of latitudinal differential rotation as a possible cause of weakened magnetic braking of solar-type stars
• Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses
• The influence of metallicity on a combined stellar and disk evolution
• Revisiting the Red-giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• Exploring the Observability of Surviving Companions of Stripped-Envelope Supernovae: A Case Study of Type Ic SN 2020oi
• Mutual Inclination of Ultra-Short-Period Planets with Time Varying Stellar J2-moment
• Characterising abundance-age relations of GALAH stars using oxygen-enhanced stellar models
• Search for ${}^{22}$Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes
• Occurrence rate of hot Jupiters orbiting red giant stars
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• 4FGL J1120.0-2204: A Unique Gamma-ray Bright Neutron Star Binary with an Extremely Low Mass Proto-White Dwarf
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The eclipsing binary HD 185912
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Discovery of a young pre-intermediate polar
• Elimination of the Blue Loops in the Evolution of Intermediate-mass Stars by the Neutrino Magnetic Moment and Large Extra Dimensions
• BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary
• Type IIP Supernova Progenitors III: Blue to Red Supergiant Ratio in Low Metallicity Models with Convective Overshoot
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. III. HD 8374 and HD 24546
• The future influence of six exoplanets on the envelope properties of their parent stars on the giant branches
• A search for transit timing variations in the HATS-18 planetary system
• Red giants evolutionary status determination: the complete Kepler catalog
• The Impacts of Neutron-Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison
• Magnetic Inclination Evolution of Accreting Neutron Stars in Intermediate/Low-Mass X-ray Binaries
• A multiphase study of theoretical and observed light curves of classical Cepheids in the Magellanic Clouds
• Polygram Stars: Resonant Tidal Excitation of Fundamental Oscillation Modes in Asynchronous Stellar Coalescence
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• The composition of massive white dwarfs and their dependence on the C-burning modeling
• The Betelgeuse Project III: Merger Characteristics
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• A Framework for Relative Biosignature Yields from Future Direct Imaging Missions
• Towards early-type eclipsing binaries as extragalactic milestones: II. NLTE spectral analysis and stellar parameters of the detached O-type system OGLE-LMC-ECL-06782 in the LMC
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
• A binary with a $\delta$~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821
• Unraveling the origin of giant exoplanets: Observational implications of convective mixing
• A closer look at the $pp$-chain reaction in the Sun: Constraining the coupling of light mediators to protons
• Heavy Dark Matter in White Dwarfs: Multiple-Scattering Capture and Thermalization
• Inferring the progenitor mass-kinetic energy relation of stripped-envelope core-collapse supernovae from nebular spectroscopy
• The Influence of Disk Composition on the Evolution of Stars in the Disks of Active Galactic Nuclei
• Photodynamical Modeling of the Fascinating Eclipses in the Triple-Star System KOI-126
• Evolutionary and Observational Consequences of Dyson Sphere Feedback
• Simulating a stellar contact binary merger -- I. Stellar models
• On asymmetric dark matter constraints from the asteroseismology of a subgiant star
• One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors
• Optical Appearance of Eccentric Tidal Disruption Events
• Orbital Dynamics and the Evolution of Planetary Habitability in the AU Mic System
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
• Tidally excited oscillations in hot white dwarfs
• The Effects of Metallicity on Convective Overshoot Behaviour in Models of delta Scuti Variable Stars
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• On period distribution of RR Lyr type variables in the globular cluster M3
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• Uncovering the chemical structure of the pulsating low-mass white dwarf SDSS J115219.99+024814.4
• Minimum Orbital Periods of H-Rich Bodies
• Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main sequence stars
• Detached Eclipsing Binaries in Compact Hierarchical Triples: Triple-lined systems BD+44 2258 and KIC 06525196
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• Novae: An Important Source of Lithium in the Galaxy
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae
• Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries
• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• Evolution of Rotating 25 M${}_{\odot }$ Population III star: Physical Properties and Resulting Supernovae
• The effect of aspherical stellar wind of giant stars on the symbiotic channel of type Ia supernovae
• Magnetic Archaeology of Early-Type Stellar Dynamos
• Pulsational Pair-instability Supernovae. II. Neutrino Signals from Pulsations and their Detection by Terrestrial Neutrino Detectors
• Simulating the deposition of angular momentum by jets in common envelope evolution
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Period Change Rates of Large Magellanic Cloud Cepheids using MESA
• Testing tidal theory using Gaia binaries: the red giant branch
• Searching for solar-like oscillations in pre-main sequence stars using APOLLO
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
• Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri
• The Formation of Discs in the Interior of AGB Stars from the Tidal Disruption of Planets and Brown Dwarfs
• The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary
• Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts
• Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
• Measuring solar neutrinos over Gigayear timescales with Paleo Detectors
• Optical color of Type Ib and Ic supernovae and implications for their progenitors
• Close encounters of black hole - star binaries with stellar-mass black holes
• WR + O binaries as probes of the first phase of mass transfer
• Refractory and Volatile Species in the UV-to-IR Transmission Spectrum of Ultra-hot Jupiter WASP-178b with HST and JWST
• Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
• Why hot Jupiters can be large but not too large
• Modified Gravity and the Flux-weighted Gravity-Luminosity Relationship of Blue Supergiant Stars
• Type Ia supernova ejecta-donor interaction: explosion model comparison
• A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
• Mixing via Thermocompositional Convection in Hybrid C/O/Ne White Dwarfs
• Mixing fraction in classical novae
• Dark Matter-admixed Rotating White Dwarfs as Peculiar Compact Objects
• On the Anti-Correlation between Duration and Redshift in Gamma-ray Bursts
• Crust Cooling Models are Insensitive to the Crust-Core Transition Pressure for Realistic Equations of State
• Parasite common envelope evolution by triple-star systems
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• Probing red-supergiant atmospheres and winds with early-time high-cadence high-resolution type II supernova spectra
• SCExAO/CHARIS Direct Imaging of A Low-Mass Companion At A Saturn-Like Separation from an Accelerating Young A7 Star
• Effect of Rotation on Wave Mixing in Intermediate Mass Stars
• The Impact of Tidal Migration of Hot Jupiters on the Rotation of Sun-like Main-sequence Stars
• Distribution and evolution of Li abundance in red clump stars can be explained by the internal gravity waves
• Hot Jupiter engulfment by a red giant in 3D hydrodynamics
• Relevance of the small frequency separation for asteroseismic stellar age, mass, and radius. A statistical investigation for main-sequence low-mass stars
• Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars
• Gamma-Ray Light Curves and Spectra of Classical Novae
• Thermonuclear 17O(n,gamma)18O reaction rate and its astrophysical implications
• ELM of ELM-WD: An extremely low mass hot star discovered in LAMOST survey
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Dynamical Tides in Eccentric Binaries Containing Massive Main-Sequence Stars: Analytical Expressions
• Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge
• Enhanced mass-loss rate evolution of stars with $\gtrsim 18M_{\odot }$ and missing optically-observed type II core-collapse supernovae
• Impact of central mixing scheme and nuclear reaction network on the extent of convective cores
• Semi-Analytical Expression of G-Mode Period Spacing: The Case of Brunt-Väisälä Frequency with Not a Jump But a Ramp
• Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations
• A catalog of new slowly pulsating B-type stars
• Overshooting in the core helium burning stage of a $30M_{\odot }$ star using the $k$-$\omega$ model
• 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
• Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity
• What governs the spin distribution of very young < 1 Myr low mass stars
• Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
• Long-term evolution of post-explosion Helium-star Companions of Type Iax Supernovae
• Weakly-Supervised Anomaly Detection in the Milky Way
• Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
• Resonant Mode Coupling in $\delta$ Scuti Stars
• Rotational and pulsational variability in the TESS light curve of HD27463
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations
• Near-Core Acoustic Glitches are Not Oscillatory: Consequences for Asteroseismic Probes of Convective Boundary Mixing
• Low energy core collapse supernovae in the frame of the jittering jets explosion mechanism
• The mass distribution of the first stars can be determined via the 21-cm signal
• Feeding post core collapse supernova explosion jets with an inflated main sequence companion
• Investigation of near-contact semi-detached binary W UMi through observations and evolutionary models
• Vetting the Lobster Diagram: Searching for Unseen Companions in Wide Binaries using NASA Space Exoplanet Missions
• Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
• VFTS 243 as predicted by the BPASS fiducial models
• The Evolution of Binaries Embedded Within Common Envelopes
• The imprint of convection on Type I X-ray bursts: Pauses in photospheric radius expansion lightcurves
• Non-linear Three-mode Coupling of Gravity Modes in Rotating Slowly Pulsating B Stars: Stationary Solutions and Modeling Potential
• Moving and Reactive Boundary Conditions in Moving-Mesh Hydrodynamics
• Two's a crowd? Characterising the effect of photometric contamination on the extraction of the global asteroseismic parameter ${\nu }_{\text{max}}$ in red-giant binaries
• The Secular Periodic Evolution of X-ray Quasi-periodic Eruptions Driven by Star-disc Collisions
• Multi-wavelength Photometric Study of RR Lyrae Variables in the Globular Cluster NGC 5272 (Messier 3)
• Carbon Isotope Ratios in M10 Giants
• The Role of Strong Gravity and the Nuclear Equation of State on Neutron-Star Common-Envelope Accretion
• Ultraluminous X-ray sources with He star companions
• Convective Mixing: The Formation Channel of Li-rich Giants
• Anomalous orbital expansion of low-mass X-ray binary 2A 1822-371: the existence of a circumbinary disk?
• Monte Carlo Radiation Transport for Astrophysical Transients Powered by Circumstellar Interaction
• Hydrogen-free Wolf-Rayet stars: Helium stars with envelope-inflation structure and rotation
• Validating Stellar Abundance Measurements from Multi-Resolution Spectroscopy
• Common envelope jets supernova with thermonuclear outburst progenitor for the enigmatic supernova remnant W49B
• Measuring mass transfer of AM CVn binaries with a space-based gravitational wave detector
• Observational Signatures of Carbon-Oxygen White Dwarf Merger Remnants
• Tidal synchronization trapping in stars and planets with convective envelopes
• A new long gamma-ray burst formation pathway at solar metallicity
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
• Searching for Hot Water World Candidates with CHEOPS: Refining the radii and analysing the internal structures and atmospheric lifetimes of TOI-238 b and TOI-1685 b
• Tidal disruption rate suppression by the event horizon of spinning black holes
• Laminar Flame Speeds in Degenerate Oxygen-Neon Mixtures
• Oscillations of red giant stars with magnetic damping in the core. I. Dissipation of mode energy in dipole-like magnetic fields
• HIP 15429: A newborn Be star on an eccentric binary orbit
• Magnetic Webs in Stellar Radiative Zones
• The core degenerate scenario for the type Ia supernova SN 2020eyj
• Type IIP Supernova Progenitors II: Stellar Mass and Obscuration by the Dust in the Circumstellar Medium
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• Differential Rotation in Convective Envelopes: Constraints from Eclipsing Binaries
• The C/N ratio from FUV spectroscopy as a constraint upon the past evolution of HS0218+3229
• The Formation of Bimodal Dust Species in Nova Ejecta
• Characterising the AGB bump and its potential to constrain mixing processes in stellar interiors
• Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests
• The ESO UVES/FEROS Large Programs of TESS OB pulsators. II. On the physical origin of macroturbulence
• On the Formation of SS433
• 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
• Non-standard modeling of a possible blue straggler star, KIC 11145123
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Uncovering the ultimate planet impostor. An eclipsing brown dwarf in a hierarchical triple with two evolved stars
• WD mass and orbital period relation of sdB + He WD binaries
• Evolution and pulsations of population I post-AGB stars
• Period-Colour and Amplitude-Colour relations for OGLE-$\delta$ Scuti stars in the Galactic Bulge and LMC
• Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
• Planet-star interactions with precise transit timing. IV. Probing the regime of dynamical tides for GK host stars
• Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• Giant planet formation via pebble accretion across different stellar masses
• The population of Galactic supernova remnants in the TeV range
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Dark Kinetic Heating of Exoplanets and Brown Dwarfs
• Pre-supernova outbursts by core magnetic activity
• Hydrodynamic simulations of WD-WD mergers and the origin of RCB stars
• Interior rotation modelling of the $\beta$ Cep pulsator HD 192575 including multiplet asymmetries
• Double eclipsing binary system KIC 3832716
• Mixed-mode coupling in the Red Clump I. Standard single star models
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• Asteroseismology of the pre-main-sequence $\delta$ Scuti pulsator IP Persei
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?
• Astrophysical Parameter Inference on Accreting White Dwarf Binaries using Gravitational Waves
• Where has all the $r$-process gone? Timescales for GRB-Kilonovae to Enrich their Host Galaxies
• V1082-Sgr: A magnetic cataclysmic variable with a lobe-filling companion star
• The Red Supergiant Progenitor of the Type II Supernova 2024abfl
• A Photometric, Spectroscopic, and Apsidal Motion Analysis of the F-type Eclipsing Binary BW Aquarii from K2 Campaign 3
• Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
• Suggested magnetic braking prescription derived from field complexity fails to reproduce the cataclysmic variable orbital period gap
• 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 Heating and Pulsations of V386 Serpentis after its 2019 Dwarf Nova Outburst
• Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars
• SN 2016iyc: A Type IIb supernova arising from a low-mass progenitor
• KIC 12268220: A $\delta$ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System
• The pre-SN activity as a possible explanation of the peculiar properties of Type IIP Supernova 2009kf
• The First High-Contrast Images of X-Ray Binaries: Detection of Candidate Companions in the $\gamma$ Cas Analog RX J1744.7$-$2713
• Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
• He-shell flashes on the surface of oxygen-neon white dwarfs
• Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra
• Light Curves and Event Rates of Axion Instability Supernovae
• Optical and spectral observations and hydrodynamic modelling of Type IIb Supernova 2017gpn
• Observational Properties of 155 $\beta$ Cephei pulsating variable stars
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• Capture rate of weakly interacting massive particles (WIMPs) in binary star systems
• A revisit to the enigmatic variable star 21 Comae
• Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
• Eccentric grazing envelope evolution towards type IIb supernova progenitors
• Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models
• Exploring the convective core of the high-amplitude $\delta$ Scuti star TIC 120857354 with asteroseismology
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• Photometric properties and stellar parameters of the rapidly rotating magnetic early-B star HD 345439
• Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae
• Photometric variability of blue straggler stars in M67 with TESS and K2
• Convective dynamos of black widow companions
• The Small Separation A-Star Companion Population: First Results with CHARA/MIRC-X
• Rapid expansion of red giant stars during core helium flash by waves propagation to the envelope and implications to exoplanets
• Age and convective core overshooting calibrations in CPD-54 810 binary system. Statistical investigation on the solution robustness
• Mapping the Milky Way in 5-D with 170 Million Stars
• Converged simulations of the nozzle shock in tidal disruption events
• X-ray binaries in M51 I: catalog and statistics
• The effects of Thomson scattering and chemical mixing on early-time light curves of double peaked type IIb supernovae
• In search of gravity mode signatures in main sequence solar-type stars observed by Kepler
• Can the Cosmological Dilation Explain the Skewness in the Gamma-Ray Burst Duration Distribution?
• A List of 49 New Stellar Twins from the Kepler Catalog of Eclipsing Binary Stars
• Mass transfer of low-mass binaries and chemical anomalies among unevolved stars in globular clusters
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• Stellar rotation and its connection to the evolution of hydrogen-dominated atmospheres of exoplanets
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• TIC 5724661: A Long-Period Binary with a Pulsating sdB Star and $\delta$ Scuti Variable
• The efficiency of mixed modes for angular momentum transport
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• Axion spectra and the associated x-ray spectra of low-mass stars
• Discovery of resonating integration modes in triple-mode high-amplitude $\delta$ Scuti stars: A new evolutionary phase indicator
• Constraining dark photon properties with Asteroseismology
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
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• Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215.82+111745.0: a model with $p$-mode pulsations consistent with the observations
• Asteroseismology: Looking for axions in the red supergiant star Alpha Ori
• Evolutionary and Observational Properties of Red Giant Acoustic Glitch Signatures
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• Tidally distorted barytropes and their Roche limits, with application to WASP-12b
• MAISTEP -- a new grid-based machine learning tool for inferring stellar parameters I. Ages of giant-planet host stars
• Simulating the outcome of binary neutron star merger in common envelope jets supernovae
• Spallation-altered accreted compositions for X-ray bursts: Impact on ignition conditions and burst ashes
• Sodium enhancement in evolved cataclysmic variables
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• The Initial Magnetic Field Distribution in AB Stars
• The impact of rotation on the stochastic excitation of stellar acoustic modes in solar-like pulsators
• Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores
• The coevolution of migrating planets and their pulsating stars through episodic resonance locking
• Gravity modes on rapidly rotating accreting white dwarfs and their variation after dwarf novae
• A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources
• Residual eccentricity of an Earth-like planet orbiting a red giant Sun
• Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur
• Impacts of the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ reaction rate on ${}^{56}\mathrm{Ni}$ nucleosynthesis in pair-instability supernovae
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
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• Further constraints on Jupiter's primordial structure
• The convective kissing instability in low-mass M-dwarf models: convective overshooting, semi-convection, luminosity functions, surface abundances and star cluster age dating
• Exploring the internal rotation of the extremely low-mass He-core white dwarf GD 278 with TESS asteroseismology
• The Effect of Dark Matter on Stars at the Galactic Center: The Paradox of Youth Problem
• Younger age for the oldest magnetic white dwarfs
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• Binary stellar evolution yields in galactic chemical evolution calculations
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• The evolutionary and asteroseismic imprints of mass accretion. The 10 M${}_{\odot }$ $\beta$ Cep case study
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• Structure and evolution of a tidally heated star
• A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC
• The theoretical pulsation spectra of hot B subdwarfs. Static and evolutionary STELUM models
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• Local two-dimensional simulations of the ignition of a helium shell detonation on a white dwarf by an impacting stream
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• Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
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• Exploring the small-scale magnetic fields of the solar analog KIC 8006161 using asteroseismology
• Testing the sources of the peculiar abundances in globular clusters
• Seismology and diffusion of ultramassive white dwarf magnetic fields
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• The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• On the effect of pulsar evaporation on the cooling of white dwarfs
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon
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• Empirical Relations for the Sensitivities of Solar-like Oscillations to Magnetic Perturbations
• Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
• Off-centre convective zones in mass accreting stellar models
• Solar models with protosolar accretion and turbulent mixing
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Kepler Binary Stars in NGC 6819 Open Cluster: KIC 5113146 and KIC 5111815
• Twenty-three New Heartbeat Star Systems Discovered Based on TESS Data
• Three-component Phase Separation for Ultramassive White Dwarf Models
• A Trio of Giant Planets Orbiting Evolved Star HD 184010
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• Radial pulsations of stars on the stage of the final helium flash
• An irradiated-Jupiter analogue hotter than the Sun
• A Search For Pulsations in the Optical Light Curve of the Nova ASASSN-17hx
• Planetary Dynamos in Evolving Cold Gas Giants
• White dwarf eccentricity fluctuation and dissipation by AGB convection
• Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology
• Constraining Axions with ZTF J1901+1458
• Nonlinear tidal excitation of super-harmonic gravity waves in main-sequence stars in binary and exoplanetary systems
• Impact of Asymmetrical Mass Ejection from Proto-White Dwarfs on the Properties of Binary Millisecond Pulsars
• Analyses of Hydrogen-stripped core-collapse supernovae using MOSFiT and MESA based tools
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Digital Infrastructure in Astrophysics
• Core-collapse supernova from a possible progenitor star of 100 M${}_{\odot }$
• Where to find over-massive brown dwarfs: new benchmark systems for binary evolution
• Evolution and period change in RR Lyr variables of the globular cluster M 3
• A Close-in Planet Orbiting Giant Star HD 167768
• On the Geometry of the Near-Core Magnetic Field in Massive Stars
• On rare core collapse supernovae inside planetary nebulae
• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
• Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
• Binary Stars Approaching Supermassive Black Holes: Hydrodynamics of Stellar Collisions, Mass Fallback and Partial TDEs
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Type Ia Supernovae from First-generation Stars
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation
• The Energy Sharing Timescale in an Analytic Framework for Common Envelope Hydrodynamics
• Impact of Simultaneous Stellar Modeling Uncertainties on the Tip of the Red Giant Branch for Axion-Election Coupling
• Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729
• A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters
• Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
• The depletion of the red supergiant envelope radiative zone during common envelope evolution
• 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
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Light Axion Emission and the Formation of Merging Binary Black Holes
• A solution to the tension of burning on neutron stars and nuclear physics
• Asteroseismology of four eccentric double-lined spectroscopic eclipsing binaries
• Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars
• Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
• Magnetized oscillatory double-diffusive convection
• Extraction of Physical Parameters of RRab Variables using Neural Network based Interpolator
• Evolution of a Long-Lived Deep-Seated Main-Sequence Magnetic Field During White Dwarf Cooling
• Explosions of pulsating red supergiants: a natural pathway for the diversity of Type II-P/L supernovae
• Onset of common envelope evolution during a core helium flash by rapid envelope expansion
• Good things come to those who wait: Watching donor stars evolve towards a mass-transfer instability
• Modeling the light curve of Type IIn-P SN 2005cl with red supergiant progenitors featuring pre-SN ourbursts
• 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
• Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
• 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
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• Partial, zombie, and full tidal disruption of stars by supermassive black holes
• Stellar response after stripping as a model for common-envelope outcomes
• The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars
• Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
• Pre-Supernova (Anti)Neutrino Emission Due to Weak-Interaction Reactions with Hot Nuclei
• Helium enrichment during classical nova outbursts
• 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?
• Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
• Foam: A Python package for forward asteroseismic modelling of gravity modes
• Irradiation effect and binary radio pulsars with giant companions
• Asteroseismic stellar modelling: systematics from the treatment of the initial helium abundance
• An Alternative Formation Scenario for Uranium-rich Giants: Engulfing a Earth-like Planet
• Jet-driven active galactic nucleus feedback in galaxy formation before black hole formation
• A stringent upper limit on Be star fractions produced by binary interaction
• 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
• Searching for Low-mass Population III Stars Disguised as White Dwarfs
• Evolutionary and hydrodynamic models of short--period Cepheids
• Study of the effects of magnetic braking on the lithium abundances of the Sun and solar-type stars
• Empirical instability strip for classical Cepheids II. The Small Magellanic Cloud galaxy
• The influence of rotation and metallicity on the explodability of massive stars
• A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
• Observational Properties of $\beta$ Cephei Stars: 88 new samples discovered Based on TESS and Gaia Data
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• Advancing Globular Cluster Constraints on the Axion-Photon Coupling
• Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• Dynamical Mass Loss at the End of TP-AGB stars
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Light Curve Models of Convective Common Envelopes
• Evolved eclipsing binary systems in the Galactic bulge: Precise physical and orbital parameters of OGLE-BLG-ECL-305487 and OGLE-BLG-ECL-116218
• Exploring the physical properties of the $\gamma$ Dor binary star RX Dra with photometry and asteroseismology
• The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
• Gaia-GIC-1: An Evolving Catastrophic Planetesimal Collision Candidate
• Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
• Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
• 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
• $\delta$ Circini: A massive hierarchical triple system with an eclipsing binary
• Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars
• Patchy nightside clouds on ultra-hot Jupiters: General Circulation Model simulations with radiatively active cloud tracers
• NGC 1850 BH1 is another stripped-star binary masquerading as a black hole
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• Near-critical magnetic fields in Kepler red giants
• CY Aquarii: A Triple System with Twin Companions
• Critical Metallicity of Cool Supergiant Formation. II. Physical Origin
• Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• A Lagrangian construction of rotating stars
• Accretion induced merger leading to core collapse supernovae in old stellar populations
• A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
• Blue Loops, Cepheids, and Forays into Axions
• Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
• Sub-photospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves
• Rare events of a peculiar thermonuclear supernova that precedes a core collapse supernova
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• High-resolution spectroscopy of detached eclipsing binaries during total eclipses
• Discovery of a runaway star likely ejected by a Type Iax Supernova
• Exploring the Small-scale Magnetic Fields in the Atmosphere of HD 49385 by Asteroseismic Analysis
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• On the non-dissipative orbital evolution of a binary system comprising non-compact components with misaligned spin and orbital angular momenta
• A new sample of massive B-type contact binary candidates from the OGLE survey of the Magellanic Clouds
• Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts
• Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
• Relativistic Coulomb Screening in Pulsational Pair Instability Supernovae
• Observational imprints of tidal internal gravity wave dissipation in star-planet systems
• Damping of Oscillations in Red Giants by Resonant Mode Coupling
• Detached Shell Carbon Stars: Tracing Thermal Pulses on the Asymptotic Giant Branch
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• Photometry and preliminary modelling of Type IIb Supernova 2017gpn
• 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
• EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
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• Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
• Faint intermediate luminosity optical transients (ILOTs) from engulfing exoplanets on the Hertzsprung gap
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• 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
• Relative Importance of Convective Uncertainties
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• Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2
• Inflated Eccentric Migration of evolving gas giants II: Numerical methodology and basic concepts
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• Are There Pre-Main-Sequence/Black Hole X-ray Binaries?
• Ensemble seismic study of the properties of the core of Red Clump stars
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• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
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• Evolutionary status and fundamental parameters of the Cepheid V1033 Cyg
• Constraints on the Axion-Photon Coupling Using Stellar Modelling
• JWST observations of 47 Tucanae: I. The low-mass main sequence down to the hydrogen-burning limit
• Detailed Characterization of Heartbeat Stars and their Tidally Excited Oscillations
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• Eighteen Exoplanet Host Stars from the NPOI Data Archive
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• The bimodal distribution of donor stars in X-ray binaries
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• Chemical fingerprints of binary mass transfer in massive stars
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
• Asteroseismic Analysis of a Red Giant KIC 9145955 by Including the Small-scale Magnetic Fields in the Atmosphere
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
• The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
• Eccentricities of millisecond pulsars with intermediate-mass progenitors
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars
• Potential Habitability as a Stellar Property: Effects of Model Uncertainties and Measurement Precision
• Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
• Atmospheric mass loss and stellar wind effects in young and old systems II: Is TOI-942 the past of TOI-421 system?
• Mechanisms for magnetic braking boost and disruption: the role of irradiation-driven winds and convective turnover time spike in cataclysmic variables
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
• NGC 2004 #115: a black hole imposter containing three luminous stars
• Slow convection and fast rotation in crystallization-driven white dwarf dynamos
• Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
• Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss
• Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
• 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
• A Theoretical Study of the Structure and Elemental Abundances of HD 20794
• Convective Penetration in Early-Type Stars
• Viscous and centrifugal instabilities of massive stars
• Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid
• 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
• On the stellar core physics of the 16 Cyg binary system: constraining the central hydrogen abundance using asteroseismology
• Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
• Cyclic light variations and accretion disk evolution in the LMC eclipsing binary OGLE-LMC-DPV-062
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
• Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
• Can small-scale magnetic fields be the major cause for the near-surface effect of the solar p-mode frequencies?
• Tidal capture and repeating partial tidal disruption events of giant stars