Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation

Abstract

We update the capabilities of the open-knowledge software instrument Modules for Experiments in Stellar Astrophysics (MESA). RSP is a new functionality in MESAstar that models the non-linear radial stellar pulsations that characterize RR Lyrae, Cepheids, and other classes of variable stars. We significantly enhance numerical energy conservation capabilities, including during mass changes. For example, this enables calculations through the He flash that conserve energy to better than 0.001 %. To improve the modeling of rotating stars in MESA, we introduce a new approach to modifying the pressure and temperature equations of stellar structure, and a formulation of the projection effects of gravity darkening. A new scheme for tracking convective boundaries yields reliable values of the convective-core mass, and allows the natural emergence of adiabatic semiconvection regions during both core hydrogen- and helium-burning phases. We quantify the parallel performance of MESA on current generation multicore architectures and demonstrate improvements in the computational efficiency of radiative levitation. We report updates to the equation of state and nuclear reaction physics modules. We briefly discuss the current treatment of fallback in core-collapse supernova models and the thermodynamic evolution of supernova explosions. We close by discussing the new MESA Testhub software infrastructure to enhance source-code development.

57 pages, 57 figures; Accepted to ApJS

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• Stable mass transfer can explain massive binary black hole mergers with a high spin component
• Towards a new era in giant exoplanet characterisation
• Predictions for gravity-mode periods and surface abundances in intermediate-mass dwarfs from shear mixing and radiative levitation
• Helium Enhanced Planets Along the Upper Edge of the Radius Valley
• Convection Reconciles the Difference in Efficiencies Between Low-Mass and High-Mass Common Envelopes
• A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae
• Black widow formation by pulsar irradiation and sustained magnetic braking
• Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods
• Successive common envelope events from multiple planets
• The Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars
• Superadiabaticity and the metallicity independence of the Humphreys-Davidson limit
• Simulating highly-eccentric common envelope jets supernova (CEJSN) impostors
• Novae heat their food: mass transfer by irradiation
• LAMOST J0140355+392651: An evolved cataclysmic variable donor transitioning to become an extremely low mass white dwarf
• Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernova
• Period bouncers as detached magnetic cataclysmic variables
• Clumping and X-Rays in cooler B supergiant stars
• Evolution and final fate of massive post-common-envelope binaries
• Asteroseismic g-mode period spacings in strongly magnetic rotating stars
• Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence
• Imprint of planet formation in the deep interior of the Sun
• Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer
• Velocity limits in the thermonuclear supernova ejection scenario for hypervelocity stars and the origin of US 708
• Seismic modeling of a very young SPB star -- KIC8264293
• Evidence of a signature of planet formation processes from solar neutrino fluxes
• The first two-dimensional stellar structure and evolution models of rotating stars
• Modified Gravity and the Black Hole Mass Gap
• On the impact of relativistic gravity on the rate of tidal disruption events
• Two decades of optical timing of the shortest-period binary star system HM Cancri
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• SN 2022acko: the First Early Far-Ultraviolet Spectra of a Type IIP Supernova
• On the energy source of ultra-stripped supernovae
• WOCS 5379: Detailed Analysis of the Evolution of a Post-Mass-Transfer Blue Straggler
• Population III X-ray Binaries and their Impact on the Early Universe
• The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
• Magnetic braking with MESA evolutionary models in the single star and LMXB regimes
• Hierarchically modelling Kepler dwarfs and subgiants to improve inference of stellar properties with asteroseismology
• Convective Mixing in Gas Giant Planets with Primordial Composition Gradients
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• Forming merging double compact objects with stable mass transfer
• Explodability criteria for the neutrino-driven supernova mechanism
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• The magneto-rotational instability in massive stars
• GASTLI: An open-source coupled interior-atmosphere model to unveil gas giant composition
• A Study of Nine Triply Eclipsing Triples
• Modeling overcontact binaries, I. The effect of tidal deformation
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• A red giant branch common envelope evolution scenario for the exoplanet WD 1856 b
• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• X-Shooting ULLYSES: Massive Stars at low metallicity VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
• WIYN Open Cluster Study. LXXXVII. HST Ultraviolet Detection of Hot White Dwarf Companions to Blue Lurkers in M67
• The effect of the centrifugal acceleration on period spacings of gravito-inertial modes in intermediate-mass stars
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• The Planetary Accretion Shock. III. Smoothing-free 2.5D simulations and calculation of H alpha emission
• On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram
• Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds from ASAS-SN: Implications for Thorne-Żytkow Objects and Super-Asymptotic Giant Branch Stars
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
• A close-in giant planet escapes engulfment by its star
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• Magnetic field breakout from white dwarf crystallization dynamos
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• The Asteroseismic Imprints of Mass Transfer: A Case Study of a Binary Mass Gainer in the SPB Instability Strip
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• beta Cas: the first delta Scuti star with a dynamo magnetic field
• An Analytical Density Profile of Dense Circumstellar Medium in Type II Supernovae
• Precursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae
• Cooling Delays from Iron Sedimentation and Iron Inner Cores in White Dwarfs
• 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
• Inverse Tides in Pulsating Binary Stars
• Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion
• Modeling contact binaries, II. The effect of energy transfer
• Contamination in TESS light curves: The case of the Fast Yellow Pulsating Supergiants
• 3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
• SPYGLASS. II. The Multi-Generational and Multi-Origin Star Formation History of Cepheus Far North
• Asteroseismic Inference of Subgiant Evolutionary Parameters with Deep Learning
• A theory of mass transfer in binary stars
• The role of stellar expansion on the formation of gravitational wave sources
• 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
• Formation of black widows through ultra-compact X-ray binaries with He star companions
• Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
• 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
• Is Thermohaline Mixing the Full Story? Evidence for Separate Mixing Events near the Red Giant Branch Bump
• Mode identification in three pulsating hot subdwarfs observed with TESS satellite
• Limits on Mode Coherence in Pulsating DA White Dwarfs Due to a Non-static Convection Zone
• Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators
• Exploring the borderline between stable mass transfer and mergers in close binary evolution
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• A theoretical framework of BL Her stars. I. Effect of metallicity and convection parameters on period-luminosity and period-radius relations
• Simulating the negative jet feedback mechanism in common envelope jets supernovae
• Testing stellar evolution with asteroseismic inversions of a main sequence star harboring a small convective core
• The Pulsation Properties of $\lambda$ Bootis Stars I. The Southern TESS Sample
• The circularization timescales of late-type binary stars
• Dark matter capture and annihilation in stars: Impact on the red giant branch tip
• The eclipsing binary systems with $\delta$ Scuti component. I. KIC 10661783
• Identifying Blue Large Amplitude Pulsators from Gaia DR2 & ZTF DR3
• 3D Hydrodynamics of Pre-supernova Outbursts in Convective Red Supergiant Envelopes
• From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
• Radiative Acceleration of Dense Circumstellar Material in Interacting Supernovae
• The "Giraffe": Discovery of a stripped red giant in an interacting binary with a $\sim 2M_{\odot }$ lower giant
• Modeling R Coronae Borealis Stars: Effects of He-Burning Shell Temperature and Metallicity
• Mode Mixing and Rotational Splittings: II. Reconciling Different Approaches to Mode Coupling
• Mixed Mode Asteroseismology of Red Giant Stars Through the Luminosity Bump
• Centrifugally Driven Mass Loss and Outbursts of Massive Stars
• Hypercritical Accretion for Black Hole High Spin in Cygnus X-1
• SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
• Hydrodynamics and survivability during post-main-sequence planetary engulfment
• A systematic study of super-Eddington layers in the envelopes of massive stars
• The Effects of Asymmetric Dark Matter on Stellar Evolution I: Spin-Dependent Scattering
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star
• 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
• Observational predictions for Thorne-Żytkow objects
• Observing and modelling the young solar analogue EK Draconis: starspot distribution, elemental abundances, and evolutionary status
• A binary system in the S cluster close to the supermassive black hole Sagittarius A*
• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• 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
• Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources
• Calibration of the convective parameters in stellar pulsation hydrocodes
• An 18.9-minute Blue Large-Amplitude Pulsator Crossing the 'Hertzsprung Gap' of Hot Subdwarfs
• Sensitivity of ${}^{44}$Ti and ${}^{56}$Ni production in CCSN shock-driven nucleosynthesis to reaction rates
• Evolution of AM CVn binaries with WD donors
• 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
• Eruption of the Envelope of Massive Stars by Energy Injection with Finite Duration
• Lithium abundances in giants as a function of stellar mass: An evidence for He-flash as the source of Li enhancement in low mass giants
• A Black Hole Kicked At Birth: MAXI J1305-704
• Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters
• DY Pegasi: An SX Phoenicis Star in a Binary System with an Evolved Companion
• The IACOB project XI. No increase of mass-loss rates over the bistability region
• A "blue ring nebula" surrounding a thousands of years old stellar merger
• Calibrating angular momentum transport in intermediate-mass stars from gravity-mode asteroseismology
• Tidally Tilted Pulsations in HD 265435, a subdwarf B Star with a Close White Dwarf Companion
• SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction
• TIC 308396022: a $\delta$ Scuti--$\gamma$ Doradus hybrid with large-amplitude radial fundamental mode and regular g-mode period spacing
• R Coronae Borealis Star Evolution: Simulating 3D Merger Events to 1D Stellar Evolution Including Large Scale Nucleosynthesis
• Asteroseismology of the dip structure in period-spacings of rapidly rotating gamma Doradus stars caused by the coupling between core and envelope oscillations
• Merging binary black holes formed through double-core evolution
• Internal Gravity Waves in Massive Stars II: Frequency Analysis Across Stellar Mass
• Observational properties of 155 O- and B-type massive pulsating stars
• Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. VI. Testing a parametric formulation for the azimuthal magneto-rotational instability
• A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: possible detection of an ejected common envelope
• Dusty, Self-obscured Transients from Stellar Coalescence
• CHIPS: Complete History of Interaction-Powered Supernovae
• Orbital decay in an accreting and eclipsing 13.7 minute orbital period binary with a luminous donor
• Determining mass accretion and jet mass-loss rates in post-asymptotic giant branch binary systems
• Dissecting the microphysics behind the metallicity-dependence of massive stars radii
• A seven-Earth-radius helium-burning star inside a 20.5-min detached binary
• Fast and Slow Crystallization-driven Convection in White Dwarfs
• 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
• Rapid formation of a very massive star >50000 $M_{\odot }$ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
• Red Horizontal Branch stars: an asteroseismic perspective
• Close Encounters of Tight Binary Stars with Stellar-mass Black Holes
• Systematic investigation of the effect of 56Ni mixing in the early photospheric velocity evolution of stripped-envelope supernovae
• Stellar models with self-consistent Rosseland opacities
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• Dating young open clusters using delta Scuti stars. Results for Trumpler 10 and Praesepe
• Pulsational instability of pre-main-sequence models from accreting protostars II. Modelling echelle diagrams of $\delta$ Scuti stars without rotational splitting
• Turbulence Supported Massive Star Envelopes
• Stellar Evolution and Tidal Dissipation in REBOUNDx
• Tidal dissipation due to the elliptical instability and turbulent viscosity in convection zones in rotating giant planets and stars
• Moving-mesh radiation-hydrodynamic simulations of wind-reprocessed transients
• Asteroseismic Inference of the Central Structure in a Subgiant Star
• Asteroseismology of $\delta$ Scuti stars: emulating model grids using a neural network
• A pulsar-helium star compact binary system formed by common envelope evolution
• The stellar photosphere-hydrogen ionization front interaction in Classical Pulsators: a theoretical explanation for observed period-colour relations
• Magnetic field evolution for crystallization-driven dynamos in C/O white dwarfs
• On the feasibility of structure inversions for gravity-mode pulsators
• The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars
• Comparison between the first and second mass eruptions from progenitors of Type IIn supernovae
• Study of the low-order $\Delta \nu$-$\bar{\rho }$ relation for moderately-rotating $\delta$ Scuti stars and its impact on their characterisation
• An efficient tidal dissipation mechanism via stellar magnetic fields
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• Period Change Rates in Large Magellanic Cloud Cepheids Revisited
• The imprint of star formation on stellar pulsations
• Fundamental properties of a selected sample of Ap stars: Inferences from interferometric and asteroseismic constraints
• WOCS 4540: Detailed Analysis of a Very Long Orbital Period Blue Straggler
• The K2 M67 Study: Precise Mass for a Turnoff Star in the Old Open Cluster M67
• VLTI/GRAVITY Observations and Characterization of the Brown Dwarf Companion HD 72946 B
• Repeating Partial Tidal Encounters of Sun-like Stars Leading to their Complete Disruption
• Formation of long-period post-common-envelope binaries II. Explaining the self-lensing binary KOI 3278
• Dynamical He Flashes in Double White Dwarf Binaries
• The Symbiotic X-ray Binary IGR J16194-2810: A Window on the Future Evolution of Wide Neutron Star Binaries From Gaia
• A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
• The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds
• Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars
• The jittering jets explosion mechanism (JJEM) in electron capture supernovae
• A Transparent Window into Early-Type Stellar Variability
• KIC 7955301: a hierarchical triple system with eclipse timing variations and an oscillating red giant
• Formation and Evolution of Accreting Compact Objects
• An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models
• Lithium in coalesced non-compact stars
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• On the orbital decay of the gas giant Kepler-1658b
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• Optimal Celestial Bodies for Dark Matter Detection
• On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations
• Stochastic excitation of internal gravity waves in rotating late F-type stars: A 3D simulation approach
• Unveiling the Structure and Dynamics of Red Giants with Asteroseismology
• Tidal evolution and diffusive growth during high-eccentricity planet migration: revisiting the eccentricity distribution of hot Jupiters
• Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk II: The importance of stellar rotation
• Cooling Models for the Most Massive White Dwarfs
• Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates
• On the role of reduced wind mass-loss rate in enabling exoplanets to shape planetary nebulae
• Rotational modulation in A and F stars: Magnetic stellar spots or convective core rotation?
• An absolute mass, precise age, and hints of planetary winds for WASP-121 A and b from a JWST NIRSpec phase curve
• Tides in the high-eccentricity migration of hot Jupiters: Triggering diffusive growth by nonlinear mode interactions
• Pulsation-driven mass loss from massive stars behind stellar mergers in metal-poor dense clusters
• The evolution of catastrophically evaporating rocky planets
• Can GW231123 have a stellar origin?
• Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
• The hydrogen clock to infer the upper stellar mass
• TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence
• Platform for Probing Radiation Transport Properties of Hydrogen at Conditions Found in the Deep Interiors of Red Dwarfs
• Empirical instability strip for classical Cepheids: I. The LMC galaxy
• Connecting integrated RGB mass loss from asteroseismology and globular clusters
• A rapidly evolving high-amplitude $\delta$ Scuti star crossing the Hertzsprung Gap
• The bulk metallicity of giant planets around M stars
• To be or not to be a black hole: detailed binary population models as a sanity check
• A 5% measurement of the gravitational constant in the Large Magellanic Cloud
• The mass distribution of stars stripped in binaries: The effect of metallicity
• Three Dimensional Natures of Massive Star Envelopes
• Effects of Winds on the Optical Properties of Type Ib and Ic Supernova Progenitors
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• The effect of the adiabatic assumption on asteroseismic scaling relations for luminous red giants
• Synthesizing Spectra from 3D Radiation Hydrodynamic Models of Massive Stars Using Monte Carlo Radiation Transport
• Asteroseismic sensitivity to internal rotation along the red-giant branch
• Unraveling the evolution of hot Jupiter systems under the effect of tidal and magnetic interactions and mass loss
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• Modeling of multimode radially pulsating High-Amplitude Delta Scuti stars from the OGLE Galactic bulge sample
• Evolution of rotating massive stars with new hydrodynamic wind models
• Mass ratio, the hills mechanism, and the galactic centre S-stars
• Pulsation Analysis of High-Amplitude $\delta$ Scuti Stars with TESS
• PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03
• Tidal Dissipation in Evolved Low and Intermediate Mass Stars
• Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• 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
• Li-rich and super Li-rich giants produced by element diffusion
• Discrepant Approaches to Modeling Stellar Tides, and the Blurring of Pseudosynchronization
• Detached and Continuous Circumstellar Matter in Type Ibc Supernovae from Mass Eruption
• EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope
• Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
• Lithium in red giants: the roles of the He-core flash and the luminosity bump
• Dynamical Screening Effects on Big Bang Nucleosynthesis
• The peculiar chemical abundance of the transitional millisecond pulsar PSR J1023+0038 -- Li enhancement
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• Stellar Shocks From Dark Matter Asteroid Impacts
• Evolution of Main-Sequence-like Surviving Companions in Type Ia Supernova Remnants
• Mode Mixing and Rotational Splittings: I. Near-Degeneracy Effects Revisited
• An upper limit on the spins of merging binary black holes formed through binary evolution
• The formation of the magnetic symbiotic star FN Sgr
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• 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
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Frequency analysis of KIC 1573174 : shedding light on the nature of HADS stars
• Unveiling complex magnetic field configurations in red giant stars
• Whispering in the dark: Faint X-ray emission from black holes with OB star companions
• Comparing Moment-Based and Monte Carlo Methods of Radiation Transport Modeling for Type II-Plateau Supernova Light Curves
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at $\approx$2 AU
• Origin and Evolution of Angular Momentum of Class II Disks
• Transition of latitudinal differential rotation as a possible cause of weakened magnetic braking of solar-type stars
• 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 Pre-main Sequence: Challenges and Prospects for Asteroseismology
• Precise Evolutionary Asteroseismology of High-Amplitude δ Scuti Star AE Ursae Majoris
• Populations of evolved massive binary stars in the Small Magellanic Cloud II: Predictions from rapid binary evolution
• Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• Discovery, TESS Characterization, and Modeling of Pulsations in the Extremely Low Mass White Dwarf GD 278
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• Discovery of a binary-origin classical Cepheid in a binary system with a 59-day orbital period
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• 4FGL J1120.0-2204: A Unique Gamma-ray Bright Neutron Star Binary with an Extremely Low Mass Proto-White Dwarf
• 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
• Mutual Inclination of Ultra-Short-Period Planets with Time Varying Stellar J2-moment
• 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
• Photometric White Dwarf Rotation
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The eclipsing binary HD 185912
• The influence of metallicity on a combined stellar and disk evolution
• The Maximum Black Hole Mass at Solar Metallicity
• Temperature dependent convective parameters for RRc 1D-models
• Occurrence rate of hot Jupiters orbiting red giant stars
• Revisiting the Red-giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters
• Exploring the Observability of Surviving Companions of Stripped-Envelope Supernovae: A Case Study of Type Ic SN 2020oi
• Search for ${}^{22}$Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes
• Characterising abundance-age relations of GALAH stars using oxygen-enhanced stellar models
• Orbital Dynamics and the Evolution of Planetary Habitability in the AU Mic System
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. III. HD 8374 and HD 24546
• The binary evolution of SAX J1808.4-3658: Implications of an evolved donor star
• BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary
• Tidally excited oscillations in hot white dwarfs
• On asymmetric dark matter constraints from the asteroseismology of a subgiant star
• Discovery of a young pre-intermediate polar
• Simulating a stellar contact binary merger -- I. Stellar models
• A Framework for Relative Biosignature Yields from Future Direct Imaging Missions
• The future influence of six exoplanets on the envelope properties of their parent stars on the giant branches
• A model for spin-orbit commensurability and synchronous starspot activity in stars with close-by planets
• The composition of massive white dwarfs and their dependence on the C-burning modeling
• Evolutionary and Observational Consequences of Dyson Sphere Feedback
• A search for transit timing variations in the HATS-18 planetary system
• The near-core rotation of HD 112429: a gamma Doradus star with TESS photometry and legacy spectroscopy
• Inferring the progenitor mass-kinetic energy relation of stripped-envelope core-collapse supernovae from nebular spectroscopy
• Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
• Unraveling the origin of giant exoplanets: Observational implications of convective mixing
• Elimination of the Blue Loops in the Evolution of Intermediate-mass Stars by the Neutrino Magnetic Moment and Large Extra Dimensions
• Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
• A multiphase study of theoretical and observed light curves of classical Cepheids in the Magellanic Clouds
• Magnetic Inclination Evolution of Accreting Neutron Stars in Intermediate/Low-Mass X-ray Binaries
• Rotational Variation Allows for Narrow Age Spread in the Extended Main Sequence Turnoff of Massive Cluster NGC 1846
• Towards early-type eclipsing binaries as extragalactic milestones: II. NLTE spectral analysis and stellar parameters of the detached O-type system OGLE-LMC-ECL-06782 in the LMC
• Magnetohydrodynamic simulations of A-type stars: Long-term evolution of core dynamo cycles
• One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
• Heavy Dark Matter in White Dwarfs: Multiple-Scattering Capture and Thermalization
• Optical Appearance of Eccentric Tidal Disruption Events
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• The Influence of Disk Composition on the Evolution of Stars in the Disks of Active Galactic Nuclei
• Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main sequence stars
• Galactic population of black holes in detached binaries with low-mass stripped helium stars: the case of LB-1 (LS~V+22~25)
• Refractory and Volatile Species in the UV-to-IR Transmission Spectrum of Ultra-hot Jupiter WASP-178b with HST and JWST
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries
• Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
• Optical color of Type Ib and Ic supernovae and implications for their progenitors
• Simulating the deposition of angular momentum by jets in common envelope evolution
• Minimum Orbital Periods of H-Rich Bodies
• Effects of a local physics change on the SH0ES determination of $H_0$
• Period Change Rates of Large Magellanic Cloud Cepheids using MESA
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• Improved asteroseismic inversions for red-giant surface rotation rates
• The Effects of Metallicity on Convective Overshoot Behaviour in Models of delta Scuti Variable Stars
• Measuring solar neutrinos over Gigayear timescales with Paleo Detectors
• Close encounters of black hole - star binaries with stellar-mass black holes
• Magnetic Archaeology of Early-Type Stellar Dynamos
• Uncovering the chemical structure of the pulsating low-mass white dwarf SDSS J115219.99+024814.4
• Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae
• Testing tidal theory using Gaia binaries: the red giant branch
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• The Formation of Discs in the Interior of AGB Stars from the Tidal Disruption of Planets and Brown Dwarfs
• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• Novae: An Important Source of Lithium in the Galaxy
• A model of anisotropic winds from rotating stars for evolutionary calculations
• Searching for solar-like oscillations in pre-main sequence stars using APOLLO
• Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
• Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Confirmation of Monoperiodicity Above 20 Seconds for Two Blue Large-Amplitude Pulsators
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Thermonuclear 17O(n,gamma)18O reaction rate and its astrophysical implications
• Physical properties of the eclipsing binary KIC 9851944 and analysis of its tidally-perturbed p- and g-mode pulsations
• Effect of Rotation on Wave Mixing in Intermediate Mass Stars
• Self-consistent method to extract non-linearities from pulsating stars light curves I. Combination frequencies
• SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures
• Asteroseismic age constraints on the open cluster NGC 2477 using oscillating stars identified with TESS FFI
• A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
• Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars
• Why hot Jupiters can be large but not too large
• Modelling stars with Gaussian Process Regression: Augmenting Stellar Model Grid
• Applications of Stellar Population Synthesis in the Distant Universe
• The Impact of Tidal Migration of Hot Jupiters on the Rotation of Sun-like Main-sequence Stars
• Semi-Analytical Expression of G-Mode Period Spacing: The Case of Brunt-Väisälä Frequency with Not a Jump But a Ramp
• On the Anti-Correlation between Duration and Redshift in Gamma-ray Bursts
• ELM of ELM-WD: An extremely low mass hot star discovered in LAMOST survey
• Hot Jupiter engulfment by a red giant in 3D hydrodynamics
• Parasite common envelope evolution by triple-star systems
• Gamma-Ray Light Curves and Spectra of Classical Novae
• Hydrodynamic modelling of pulsation period decrease in the Mira-type variable T UMi
• Dark Matter-admixed Rotating White Dwarfs as Peculiar Compact Objects
• Dynamical Tides in Eccentric Binaries Containing Massive Main-Sequence Stars: Analytical Expressions
• Distribution and evolution of Li abundance in red clump stars can be explained by the internal gravity waves
• Modified Gravity and the Flux-weighted Gravity-Luminosity Relationship of Blue Supergiant Stars
• Stability and pulsation of the first dark stars
• Long-term evolution of post-explosion Helium-star Companions of Type Iax Supernovae
• Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product
• VFTS 243 as predicted by the BPASS fiducial models
• Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
• A catalog of new slowly pulsating B-type stars
• The mass distribution of the first stars can be determined via the 21-cm signal
• On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations
• Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
• What governs the spin distribution of very young < 1 Myr low mass stars
• Feeding post core collapse supernova explosion jets with an inflated main sequence companion
• Multi-wavelength Photometric Study of RR Lyrae Variables in the Globular Cluster NGC 5272 (Messier 3)
• Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary
• The Secular Periodic Evolution of X-ray Quasi-periodic Eruptions Driven by Star-disc Collisions
• Near-Core Acoustic Glitches are Not Oscillatory: Consequences for Asteroseismic Probes of Convective Boundary Mixing
• The Evolution of Binaries Embedded Within Common Envelopes
• Implications of a turbulent convection model for classical Cepheids
• OGLE-GAL-ACEP-091 -- The First Known Multi-Mode Anomalous Cepheid
• Precise Fourier parameters of Cepheid Radial Velocity Curves
• Moving and Reactive Boundary Conditions in Moving-Mesh Hydrodynamics
• Non-linear Three-mode Coupling of Gravity Modes in Rotating Slowly Pulsating B Stars: Stationary Solutions and Modeling Potential
• Rotational and pulsational variability in the TESS light curve of HD27463
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
• Synthetic Spectra of Rotating Stars
• The Role of Strong Gravity and the Nuclear Equation of State on Neutron-Star Common-Envelope Accretion
• The imprint of convection on Type I X-ray bursts: Pauses in photospheric radius expansion lightcurves
• White dwarf -- red giant star binaries as Type Ia supernova progenitors: with and without magnetic confinement
• Resonant Mode Coupling in $\delta$ Scuti Stars
• Asteroseismic Inversions for Internal Sound Speed Profiles of Main-sequence Stars with Radiative Cores
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• Laminar Flame Speeds in Degenerate Oxygen-Neon Mixtures
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests
• Testing a non-local 1-equation turbulent convection model: A solar model
• Magnetic Webs in Stellar Radiative Zones
• Characterising the AGB bump and its potential to constrain mixing processes in stellar interiors
• HIP 15429: A newborn Be star on an eccentric binary orbit
• The Sun: Light Dark Matter and Sterile Neutrinos
• The ESO UVES/FEROS Large Programs of TESS OB pulsators. II. On the physical origin of macroturbulence
• Oscillations of red giant stars with magnetic damping in the core. I. Dissipation of mode energy in dipole-like magnetic fields
• On the Formation of SS433
• Tidal disruption rate suppression by the event horizon of spinning black holes
• Monte Carlo Radiation Transport for Astrophysical Transients Powered by Circumstellar Interaction
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
• Overview and Validation of the Asteroseismic Modeling Portal v2.0
• A new long gamma-ray burst formation pathway at solar metallicity
• The origin of hypervelocity white dwarfs in the merger-disruption of He-CO white dwarfs
• Convective Mixing: The Formation Channel of Li-rich Giants
• Common envelope jets supernova with thermonuclear outburst progenitor for the enigmatic supernova remnant W49B
• The core degenerate scenario for the type Ia supernova SN 2020eyj
• Observational Signatures of Carbon-Oxygen White Dwarf Merger Remnants
• Anomalous orbital expansion of low-mass X-ray binary 2A 1822-371: the existence of a circumbinary disk?
• Revealing the Fate of Exoplanet Systems: Asteroseismic Identification of Host Star in the Red Clump or Red Giant Branch
• Measuring mass transfer of AM CVn binaries with a space-based gravitational wave detector
• The C/N ratio from FUV spectroscopy as a constraint upon the past evolution of HS0218+3229
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692
• Period-Colour and Amplitude-Colour relations for OGLE-$\delta$ Scuti stars in the Galactic Bulge and LMC
• Non-standard modeling of a possible blue straggler star, KIC 11145123
• Ultraluminous X-ray sources with He star companions
• 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
• The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor
• Convective shells in the interior of Cepheid variable stars: overshooting models based on hydrodynamic simulations
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• Converged simulations of the nozzle shock in tidal disruption events
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
• Interior rotation modelling of the $\beta$ Cep pulsator HD 192575 including multiplet asymmetries
• Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• Mapping the Milky Way in 5-D with 170 Million Stars
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Spindown of massive main sequence stars in the Milky Way
• Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars
• Mixed-mode coupling in the Red Clump I. Standard single star models
• Exploring the convective core of the high-amplitude $\delta$ Scuti star TIC 120857354 with asteroseismology
• Suggested magnetic braking prescription derived from field complexity fails to reproduce the cataclysmic variable orbital period gap
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Observational Properties of 155 $\beta$ Cephei pulsating variable stars
• Dark Kinetic Heating of Exoplanets and Brown Dwarfs
• The population of Galactic supernova remnants in the TeV range
• Hydrodynamic simulations of WD-WD mergers and the origin of RCB stars
• Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers
• Pre-supernova outbursts by core magnetic activity
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• The effects of Thomson scattering and chemical mixing on early-time light curves of double peaked type IIb supernovae
• Astrophysical Parameter Inference on Accreting White Dwarf Binaries using Gravitational Waves
• 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
• Convective dynamos of black widow companions
• Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant
• In search of gravity mode signatures in main sequence solar-type stars observed by Kepler
• Photometric properties and stellar parameters of the rapidly rotating magnetic early-B star HD 345439
• Light Curves and Event Rates of Axion Instability Supernovae
• Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra
• Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models
• Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae
• 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
• Capture rate of weakly interacting massive particles (WIMPs) in binary star systems
• Asteroseismology of the heartbeat star KIC 5006817
• Evolutionary status of W Vir pulsating variables
• Weighing stars from birth to death: mass determination methods across the HRD
• The former companion of the hyper-velocity star S5-HVS1
• Eccentric grazing envelope evolution towards type IIb supernova progenitors
• Tidally distorted barytropes and their Roche limits, with application to WASP-12b
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• Simulating the outcome of binary neutron star merger in common envelope jets supernovae
• Structure and evolution of a tidally heated star
• Pre-supernova Ultra-light Axion-like Particles
• Formation of millisecond pulsar-helium star binaries
• Constraining dark photon properties with Asteroseismology
• Discovery of resonating integration modes in triple-mode high-amplitude $\delta$ Scuti stars: A new evolutionary phase indicator
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
• Local two-dimensional simulations of the ignition of a helium shell detonation on a white dwarf by an impacting stream
• The fast rise of the unusual Type IIL/IIb SN 2018ivc
• The theoretical pulsation spectra of hot B subdwarfs. Static and evolutionary STELUM models
• Impacts of the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ reaction rate on ${}^{56}\mathrm{Ni}$ nucleosynthesis in pair-instability supernovae
• Residual eccentricity of an Earth-like planet orbiting a red giant Sun
• Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores
• 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
• Effect of irradiation on the spin of millisecond pulsars
• The post-disk (or primordial) spin distribution of M dwarf stars
• Sodium enhancement in evolved cataclysmic variables
• MAISTEP -- a new grid-based machine learning tool for inferring stellar parameters I. Ages of giant-planet host stars
• Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215.82+111745.0: a model with $p$-mode pulsations consistent with the observations
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• Exploring the internal rotation of the extremely low-mass He-core white dwarf GD 278 with TESS asteroseismology
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
• A rapidly fading star as a type II obscuring intermediate luminosity optical transient (ILOT) in a triple star system
• Asteroseismology: Looking for axions in the red supergiant star Alpha Ori
• Weak or strong: coupling of mixed oscillation modes on the red-giant branch
• The efficiency of mixed modes for angular momentum transport
• Parametric models of core-helium-burning stars: structural glitches near the core
• The convective kissing instability in low-mass M-dwarf models: convective overshooting, semi-convection, luminosity functions, surface abundances and star cluster age dating
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• TIC 5724661: A Long-Period Binary with a Pulsating sdB Star and $\delta$ Scuti Variable
• Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur
• The evolutionary and asteroseismic imprints of mass accretion. The 10 M${}_{\odot }$ $\beta$ Cep case study
• A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources
• Younger age for the oldest magnetic white dwarfs
• Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
• The coevolution of migrating planets and their pulsating stars through episodic resonance locking
• A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC
• Binary stellar evolution yields in galactic chemical evolution calculations
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• Further constraints on Jupiter's primordial structure
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• The Initial Magnetic Field Distribution in AB Stars
• On the incidence rate of RR Lyrae stars with non-radial modes
• On rare core collapse supernovae inside planetary nebulae
• Shaping core dynamos in A-type stars: The role of dipolar fossil fields
• Three-component Phase Separation for Ultramassive White Dwarf Models
• The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars
• Off-centre convective zones in mass accreting stellar models
• Flare frequency in M dwarfs belonging to Young Moving Groups
• Solar models with protosolar accretion and turbulent mixing
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• Empirical Relations for the Sensitivities of Solar-like Oscillations to Magnetic Perturbations
• Tracking the Long-Term GW Phase Evolution for HM Cancri-like Binaries with LISA
• On the Geometry of the Near-Core Magnetic Field in Massive Stars
• Nonlinear tidal excitation of super-harmonic gravity waves in main-sequence stars in binary and exoplanetary systems
• Where to find over-massive brown dwarfs: new benchmark systems for binary evolution
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Review: Accretion Disk Evolution in Tidal Disruption Events
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Binary Stars Approaching Supermassive Black Holes: Hydrodynamics of Stellar Collisions, Mass Fallback and Partial TDEs
• Core-collapse supernova from a possible progenitor star of 100 M${}_{\odot }$
• Neutrinos and Asteroseismology of Stars over the Helium Flash
• Potential Tertiary Effects on the LISA Verification Binary HM Cancri
• White dwarf eccentricity fluctuation and dissipation by AGB convection
• Twenty-three New Heartbeat Star Systems Discovered Based on TESS Data
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Seismology and diffusion of ultramassive white dwarf magnetic fields
• Constraining Axions with ZTF J1901+1458
• Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA
• Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
• An irradiated-Jupiter analogue hotter than the Sun
• Constraining the Rotation Profile in a Low-Luminosity Subgiant with a Surface Rotation Measurement
• Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
• Radiative acceleration calculation methods and abundance anomalies in Am stars
• Linking solar bosonic dark matter halos and active neutrinos
• Planetary Dynamos in Evolving Cold Gas Giants
• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Solar-like oscillations and ellipsoidal variations in TESS observations of the binary 12 Boötis
• Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
• Ultrashort-period WD binaries are not undergoing strong tidal heating
• Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology
• Analyses of Hydrogen-stripped core-collapse supernovae using MOSFiT and MESA based tools
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• A stringent upper limit on Be star fractions produced by binary interaction
• 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
• Extraction of Physical Parameters of RRab Variables using Neural Network based Interpolator
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• Foam: A Python package for forward asteroseismic modelling of gravity modes
• Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
• A new framework of multidimensional pulsating stellar envelopes I.: Properties of turbulent convection in static RR Lyrae envelope models with SPHERLS
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Magnetized oscillatory double-diffusive convection
• 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
• Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
• Evolution of a Long-Lived Deep-Seated Main-Sequence Magnetic Field During White Dwarf Cooling
• Study of the effects of magnetic braking on the lithium abundances of the Sun and solar-type stars
• Accreting White Dwarfs: Effect of WD Composition on Helium Ignition During Slow Accretion
• Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Pre-Supernova (Anti)Neutrino Emission Due to Weak-Interaction Reactions with Hot Nuclei
• 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
• Explosions of pulsating red supergiants: a natural pathway for the diversity of Type II-P/L supernovae
• Probing the Axion-Nucleon Coupling with Supergiant Stars
• Magnetic dynamos powered by white dwarf superficial convection
• The depletion of the red supergiant envelope radiative zone during common envelope evolution
• Impact of Simultaneous Stellar Modeling Uncertainties on the Tip of the Red Giant Branch for Axion-Election Coupling
• Partial, zombie, and full tidal disruption of stars by supermassive black holes
• Onset of common envelope evolution during a core helium flash by rapid envelope expansion
• A Continuous Galactic Line Source of Axions: The Remarkable Case of 23Na
• A solution to the tension of burning on neutron stars and nuclear physics
• The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations
• Good things come to those who wait: Watching donor stars evolve towards a mass-transfer instability
• The Fraction of Distilled White Dwarfs with Long-Lived Habitable Zones
• Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars
• A post-common-envelope binary with double-peaked Balmer emission lines from TMTS
• The model fitting of Gaia DR3 Classical Cepheid light and radial velocity curves
• Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
• Hydrodynamic model of decaying radial oscillations in RU Cam
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Stellar response after stripping as a model for common-envelope outcomes
• The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf's code predictions
• Asteroseismic detection of an internal magnetic field in the B0.5V pulsator HD 192575
• Asteroseismology of sz lyn using multi-band high time resolution photometry from ground and space
• The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars
• Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
• Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation
• Irradiation effect and binary radio pulsars with giant companions
• Asteroseismology of low-mass stars: the balance between partial ionisation and Coulomb interactions
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Type Ia Supernovae from First-generation Stars
• Second-generation planet formation after tidal disruption from common envelope evolution
• 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
• Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
• A Lagrangian construction of rotating stars
• On the non-dissipative orbital evolution of a binary system comprising non-compact components with misaligned spin and orbital angular momenta
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• A new sample of massive B-type contact binary candidates from the OGLE survey of the Magellanic Clouds
• 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
• Can circumstellar interaction explain the strange light curve features of Type Ib/c supernovae?
• Patchy nightside clouds on ultra-hot Jupiters: General Circulation Model simulations with radiatively active cloud tracers
• Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• CY Aquarii: A Triple System with Twin Companions
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Critical Metallicity of Cool Supergiant Formation. II. Physical Origin
• Advancing Globular Cluster Constraints on the Axion-Photon Coupling
• TULIPS: a Tool for Understanding the Lives, Interiors, and Physics of Stars
• Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars
• The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Neutrinos from stars in the Milky Way
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• The influence of rotation and metallicity on the explodability of massive stars
• Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
• Double-faced white dwarfs and the magnetic inhibition of convection
• 3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors
• Accretion induced merger leading to core collapse supernovae in old stellar populations
• NGC 1850 BH1 is another stripped-star binary masquerading as a black hole
• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
• Dynamical Mass Loss at the End of TP-AGB stars
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Discovery of a runaway star likely ejected by a Type Iax Supernova
• Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects
• Near-critical magnetic fields in Kepler red giants
• Rare events of a peculiar thermonuclear supernova that precedes a core collapse supernova
• Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
• Blueshifted hydrogen emission and shock wave of RR Lyrae variables in SDSS and LAMOST
• A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• Exploring the Small-scale Magnetic Fields in the Atmosphere of HD 49385 by Asteroseismic Analysis
• Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
• 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
• $\delta$ Circini: A massive hierarchical triple system with an eclipsing binary
• 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
• Stationary accretion flow with nuclear burning
• A magnetic field detection in the massive O-type bright giant 63 Oph
• Axion Instability Supernovae
• A Theoretical Study of the Structure and Elemental Abundances of HD 20794
• Excitation and Damping of Oscillation Modes in Gaseous Planets
• 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
• Detection horizon for the neutrino burst from the stellar helium flash
• Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
• Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
• Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
• Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities
• 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
• Validation of the Gaia Early Data Release 3 parallax zero-point model with asteroseismology
• An internal heating mechanism operating in ultra-short-period planets orbiting magnetically active stars
• Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
• Slow convection and fast rotation in crystallization-driven white dwarf dynamos
• High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars
• Expectation for the MeV Gamma-Ray Emission from Pair-Instability Supernovae
• Effects of Pycnonuclear Reactions on White Dwarf Stellar Evolution
• Eccentricities of millisecond pulsars with intermediate-mass progenitors
• One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations
• The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
• 2M17091769+3127589: a mass-transfer binary with an extreme mass ratio
• Primordial black holes capture by stars and induced collapse to low-mass stellar black holes
• The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
• Formation, diffusion and accreting pollution of DB white dwarfs
• 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
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• A New Versatile Code for Gamma-Ray Monte-Carlo Radiative Transfer
• Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2
• Detailed Characterization of Heartbeat Stars and their Tidally Excited Oscillations
• NGC 2004 #115: a black hole imposter containing three luminous stars
• 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
• BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• Chemical fingerprints of binary mass transfer in massive stars
• EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
• JWST observations of 47 Tucanae: I. The low-mass main sequence down to the hydrogen-burning limit
• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
• Three-dimensional simulations of accretion disks in pre-CE systems
• Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• Effects of metallicity on mode switching in Cepheids
• Formation of black holes from He stars
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
• KIC 3868420: A high-amplitude $\delta$ Scuti-$\gamma$ Dor hybrid star crossing the Hertzsprung gap
• Huntsman may need to be irradiated
• One's loss is (not) another's gain: Isotropic re-emission destabilizes mass transfer from radiative donor stars
• Heavy dark matter in rapidly evolving massive stars
• The nature of anomalous period increase in the pulsating variable V725 Sgr
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• MESA-Web: A cloud resource for stellar evolution in astronomy curricula
• Atmospheric mass loss and stellar wind effects in young and old systems II: Is TOI-942 the past of TOI-421 system?
• Potential Habitability as a Stellar Property: Effects of Model Uncertainties and Measurement Precision
• Ensemble seismic study of the properties of the core of Red Clump stars
• Gravitational-Wave Signatures of Massive Black Hole Formation
• Constraints on the Axion-Photon Coupling Using Stellar Modelling
• Comprehensive analysis of a symbiotic candidate V503 Her
• Physical interpretation of the oscillation spectrum on the RGB and AGB
• Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
• SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host
• Apsidal motion and proximity effects in the massive binary BD+60 497
• Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA
• Detectability of compact intermediate-mass black hole binaries as low-frequency gravitational wave sources: the influence of dynamical friction of dark matter
• 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
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• Faint intermediate luminosity optical transients (ILOTs) from engulfing exoplanets on the Hertzsprung gap
• Can the Anomalous Magnetic Braking of Ap/Bp Stars Explain the Orbital Decay of Algol-type Binaries?
• Inflated Eccentric Migration of evolving gas giants II: Numerical methodology and basic concepts
• Orbital and Pulsation Analysis of 42 Heartbeat Stars Discovered in TESS Data
• Evolution of the ZTF SLRN-2020 star-planet merger
• Observational imprints of tidal internal gravity wave dissipation in star-planet systems
• Tidal capture and repeating partial tidal disruption events of giant stars
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
• Possible in situ formation of Uranus and Neptune via Pebble Accretion
• Convective Penetration in Early-Type Stars
• Viscous and centrifugal instabilities of massive stars
• Reconstruction of Cepheid Radial Velocity Curves from the shape of the V-band Light Curves
• Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
• A Multi-Planet System's Sole Super-Puff: Exploring Allowable Physical Parameters for the Cold Super-Puff HIP 41378 f
• The Cooling of Old White Dwarfs in 47 Tucanae
• Magnetic dynamos in white dwarfs -III: explaining the occurrence of strong magnetic fields in close double white dwarfs
• On the diversity of mixing and helium core masses of B-type dwarfs from gravity-mode asteroseismology
• Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
• The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars