Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure

Abstract

The evolution of rotating stars with zero-age main sequence (ZAMS) masses in the range 8 to 25 M_sun is followed through all stages of stable evolution. The initial angular momentum is chosen such that the star's equatorial rotational velocity on the ZAMS ranges from zero to ~ 70 % of break-up. Redistribution of angular momentum and chemical species are then followed as a consequence of rotationally induced circulation and instablities. The effects of the centrifugal force on the stellar structure are included. Uncertain mixing efficiencies are gauged by observations. We find, as noted in previous work, that rotation increases the helium core masses and enriches the stellar envelopes with products of hydrogen burning. We determine, for the first time, the angular momentum distribution in typical presupernova stars along with their detailed chemical structure. Angular momentum loss due to (non-magnetic) stellar winds and the redistribution of angular momentum during core hydrogen burning are of crucial importance for the specific angular momentum of the core. Neglecting magnetic fields, we find angular momentum transport from the core to the envelope to be unimportant after core helium burning. We obtain specific angular momenta for the iron core and overlaying material of 1E16...1E17 erg s. These values are insensitive to the initial angular momentum. They are small enough to avoid triaxial deformations of the iron core before it collapses, but could lead to neutron stars which rotate close to break-up. They are also in the range required for the collapsar model of gamma-ray bursts. The apparent discrepancy with the measured rotation rates of young pulsars is discussed.

62 pages, including 7 tables and 19 figures. Accepted by ApJ

References in corpus (6)

• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• Hyper-Accreting Black Holes and Gamma-Ray Bursts
• Gravitational waves from hot young rapidly rotating neutron stars
• Gravitational Radiation Instability in Hot Young Neutron Stars
• Why pulsars rotate and move: kicks at birth
• Discovery of an Ultra-fast X-ray Pulsar in the Supernova Remnant N157B

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• Gamma Ray Burst Production and Supernova Signatures in Slowly Rotating Collapsars
• Asteroseismology of the Nearby SN-II Progenitor Rigel Part II. ε-Mechanism Triggering Gravity-Mode Pulsations?
• On the asymptotic giant branch star origin of peculiar spinel grain OC2
• On The Development of Multidimensional Progenitor Models For Core-collapse Supernovae
• Explaining the differences in massive star models from various simulations
• Nuclear Burning in Collapsar Accretion Disks
• Mass discrepancy analysis for a select sample of Type II-Plateau supernovae
• The Arduous Journey to Black-Hole Formation in Potential Gamma-Ray Burst Progenitors
• Evolving R Coronae Borealis Stars with MESA
• MESA models with magnetic braking
• The Morphology and Dynamics of Jet-Driven Supernova Remnants: the Case of W49B
• The Angular Momenta of Neutron Stars and Black Holes as a Window on Supernovae
• Critical Surface for Explosions of Rotational Core-Collapse Supernovae
• Pulsars With Jets May Harbor Dynamically Important Accretion Disks
• Critical angular velocity and anisotropic mass loss of rotating stars with radiation-driven winds
• Continuous gravitational waves from Galactic neutron stars: demography, detectability and prospects
• Testing the neutrino annihilation model for launching GRB jets
• High Energy neutrino signals from the Epoch of Reionization
• Is Betelgeuse the Outcome of a Past Merger?
• Multisite campaign on the open cluster M67. III. Delta Scuti pulsations in the blue stragglers
• A study of the effect of rotational mixing on massive stars evolution: surface abundances of Galactic O7-8 giant stars
• Isochrone-cloud fitting of the extended Main-Sequence Turn-Off of young clusters
• Constraining transport of angular momentum in stars: Combining asteroseismic observations of core helium burning stars and white dwarfs
• Radio emission from the cocoon of a GRB jet: implications for relativistic supernovae and off-axis GRB emission
• A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
• Five young $\delta$ Scuti stars in the Pleiades seen with Kepler/K2
• Failure of a neutrino-driven explosion after core-collapse may lead to a thermonuclear supernova
• Chemical Mixing Induced by Internal Gravity Waves in Intermediate Mass Stars
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• Testing Self-Organized Criticality Across the Main Sequence using Stellar Flares from TESS
• MAESTROeX: A Massively Parallel Low Mach Number Astrophysical Solver
• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
• Ejecta and progenitor of the low-luminosity Type IIP supernova 2003Z
• New \textsl{s}-process Mechanism in Rapidly-Rotating Massive Pop II Stars
• The formation of black hole low-mass X-ray binaries: through case B or case C mass transfer?
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• Helium ignition in rotating magnetized CO white dwarfs leading to fast and faint rather than classical type Ia supernovae
• North-South Neutrino Heating Asymmetry in Strongly Magnetized and Rotating Stellar Cores
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• Asteroseismic test of rotational mixing in low-mass white dwarfs
• Predictions for gravity-mode periods and surface abundances in intermediate-mass dwarfs from shear mixing and radiative levitation
• Simulating X-ray bursts during a transient accretion event
• Finding the First Cosmic Explosions. IV. 90 - 140 M${}_{\odot }$ Pair-Instability Supernovae
• Observational signatures of past mass-exchange episodes in massive binaries: The case of HD 149 404
• Superadiabaticity and the metallicity independence of the Humphreys-Davidson limit
• A collapsar origin for GRB 211211A is (just barely) possible
• The Final Fate of Supermassive $M\sim 5\times 10^4{M}_{\odot }$ Pop III Stars: Explosion or Collapse?
• Rotating Stars and the Formation of Bipolar Planetary Nebulae II: Tidal Spin-up
• Diagnostic of the unstable envelopes of Wolf-Rayet stars
• The first two-dimensional stellar structure and evolution models of rotating stars
• Discovery of Variability of the Progenitor of SN 2011dh in M51 Using the Large Binocular Telescope
• The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
• The Evolution of Helium Star Plus Carbon-Oxygen White Dwarf Binary Systems and Implications for Diverse Stellar Transients and Hypervelocity Stars
• The large landscape of supernova, GRB and cocoon interactions
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• Gamma-ray bursts and Population III stars
• How much mass and angular momentum can the progenitors of carbon-enriched stars accrete?
• Role of supergiants in the formation of globular clusters
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
• The magneto-rotational instability in massive stars
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• Evolutions of stellar-mass black hole hyperaccretion systems in the center of gamma-ray bursts
• Supernovae from massive stars
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Diffusion in stellar interiors: critical tests of three numerical methods
• Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
• Critical angular momentum distributions in collapsars: quiescent periods from accretion state transitions in long gamma-ray bursts
• Monotonicity of the cores of massive stars
• Supernovae Powered by Collapsar Accretion in Gamma-Ray Burst Sources
• The role of stellar expansion on the formation of gravitational wave sources
• A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes
• The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints
• Exploring the borderline between stable mass transfer and mergers in close binary evolution
• The VLT-FLAMES Tarantula Survey XXVII. Physical parameters of B-type main-sequence binary systems in the Tarantula nebula
• Residual Carbon in Oxygen-Neon White Dwarfs and its Implications for Accretion-Induced Collapse
• High-mass eclipsing binaries: a testbed for models of interior structure and evolution -- Accurate fundamental properties and surface chemical composition for V1034 Sco, GL Car, V573 Car and V346 Cen
• The Art of Modeling Stellar Mergers and the Case of the B[e] Supergiant R4 in the Small Magellanic Cloud
• Population synthesis of young isolated neutron stars: the effect of fallback disk accretion and magnetic field evolution
• Neutrino Emission in Jet Propagation Process
• Influence of Rotation on Stellar Evolution
• A MAD Model for Gamma-Ray Burst Variability
• The evolution of single B-type stars with a large angular momentum content
• The GSF Instability and Turbulence do not Account for the Relatively Low Rotation Rate of Pulsars
• Testing a one-dimensional prescription of dynamical shear mixing with a two-dimensional hydrodynamic simulation
• Is there a mass discrepancy in the Cepheid binary OGLE-LMC-CEP0227?
• The Gravitational Wave Signature of Core-Collapse Supernovae
• Towards a unified model of stellar rotation II: Model-dependent characteristics of stellar populations
• The sculpting of rectangular and jet-like morphologies in supernova remnants by anisotropic equatorially-confined progenitor stellar winds
• A systematic study of super-Eddington layers in the envelopes of massive stars
• Metallicity dependence of turbulent pressure and macroturbulence in stellar envelopes
• Centrifugally Driven Mass Loss and Outbursts of Massive Stars
• Convection and rotation boosted prescription of magnetic braking: application to the formation of extremely low-mass white dwarfs
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Numerical approaches for multidimensional simulations of stellar explosions
• Calibrating angular momentum transport in intermediate-mass stars from gravity-mode asteroseismology
• 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
• The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: spectroscopy, orbital analysis, formation, and evolution
• Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors
• On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres
• A Spectroscopic and Photometric Investigation of the Mercury-Manganese Star KIC 6128830
• Young Clusters in the Magellanic Clouds II
• Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
• A comprehensive study of young B stars in NGC 2264: I. Space photometry and asteroseismology
• Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. VI. Testing a parametric formulation for the azimuthal magneto-rotational instability
• Differential Rotation in a 3D Simulation of Oxygen Shell Burning
• Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
• Aluminium-26 from massive binary stars III. Binary stars up to core-collapse and their impact on the early Solar System
• Observational signatures of past mass-exchange episodes in massive binaries: The case of LSS 3074
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• On the photometric signature of fast rotators
• Pre-explosion dynamo in the cores of massive stars
• Induced differential rotation and mixing in asynchronous binary stars
• Turbulent transport by diffusive stratified shear flows: from local to global models. III. A closure model
• A versatile numerical method for obtaining structures of rapidly rotating baroclinic stars: self-consistent and systematic solutions with shellular-type rotation
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• Rapidly rotating neutron star progenitors
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Saturation of the f-mode instability in neutron stars: II. Applications and results
• The spins of stripped B stars support magnetic internal angular momentum transport
• Spindown of massive rotating stars
• Nucleosynthesis in the outflows associated with accretion disks of Type II collapsars
• A strong neutron burst in jet-like supernovae of spinstars
• Looking deep into the Cat's Eye: Structure and rotation in the fast wind of the PN central star of NGC6543
• Formation of long-period post-common-envelope binaries II. Explaining the self-lensing binary KOI 3278
• Constraining the r-mode saturation amplitude from a hypothetical detection of r-mode gravitational waves from a newborn neutron star - sensitivity study
• Evolution and Nucleosynthesis of Very Massive Stars
• Rotation and Magnetism of Massive Stellar Cores
• The Three-Dimensional Collapse of a Rapidly Rotating 16 $M_{\odot }$ Star
• A Study of Wolf-Rayet stars Formed via Chemically Homogeneous Evolution
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• Lithium in coalesced non-compact stars
• Turbulent Mixing on Helium-Accreting White Dwarfs
• Can very massive Population III stars produce a super-collapsar?
• Physics of rotation in stellar models
• Computational Models of Stellar Collapse and Core-Collapse Supernovae
• The Regulated NiCu Cycles with the new ${}^{57}$Cu(p,$\gamma$)${}^{58}$Zn reaction rate and the Influence on Type-I X-Ray Bursts: GS 1826$-$24 Clocked Burster
• Neutron stars formation and Core Collapse Supernovae
• Extended supernova shock breakout signals from inflated stellar envelopes
• The hydrogen clock to infer the upper stellar mass
• Off-axis synchrotron light curves from full-time-domain moving-mesh simulations of jets from massive stars
• Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
• Structure and evolution of rotationally and tidally distorted stars
• Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars
• The formation of the magnetic symbiotic star FN Sgr
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Angular momentum transport near convective-core boundaries of Gamma Doradus stars
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• The effects of rotation on massive star spectroscopic observables
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase
• Neutron star binaries and long duration gamma-ray bursts
• 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
• Presupernova Structure of Massive Stars
• Stochastic Core Spin-Up in Massive Stars -- Implications of 3D Simulations of Oxygen Shell Burning
• Small-Scale Dynamo in Stably Stratified Turbulence
• The radiative zone of the Sun and the tachocline: stability of baroclinic patterns of differential rotation
• Scenarios to explain extreme Be depletion in solar-like stars: accretion or rotation effects ?
• Neutrino oscillations in magnetically driven supernova explosions
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Metallicity-Suppressed Collapsars Cannot be the Dominant r-Process Source in the Milky Way
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• Photometric White Dwarf Rotation
• The Maximum Black Hole Mass at Solar Metallicity
• Galactic Population Synthesis of Radioactive Nucleosynthesis Ejecta
• Rotational mixing in carbon-enhanced metal-poor stars with s-process enrichment
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• Fallback onto Kicked Neutron Stars and its Effect on Spin-Kick Alignment
• 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
• BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary
• The Betelgeuse Project III: Merger Characteristics
• On large-scale dynamos with stable stratification and the application to stellar radiative zones
• Effects of the core-collapse supernova ejecta impact on a rapidly rotating massive companion star
• Implications of Elemental Abundances in Dwarf Spheroidal Galaxies
• Uncovering the chemical structure of the pulsating low-mass white dwarf SDSS J115219.99+024814.4
• Spatial distribution of radionuclides in 3D models of SN 1987A and Cas A
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
• Spin evolution of neutron stars in wind-fed high mass X-ray binaries
• Thermohaline mixing in low-mass giants
• He abundance of Dense Circumstellar Clumps in the Cassiopeia A Supernova Remnant
• Differentially Rotating White Dwarfs I: Regimes of Internal Rotation
• A model of anisotropic winds from rotating stars for evolutionary calculations
• Does energy of type IIP supernovae depends on stellar mass?
• Period Change Rates of Large Magellanic Cloud Cepheids using MESA
• How Efficient is Rotational Mixing in Massive Stars ?
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• Analytic approximations for massive close post-mass transfer binary systems
• BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
• Metal-enriched Pair-instability supernovae: Effects of rotation
• Nucleosynthesis from massive stars 50 years after B2FH
• Asteroseismic age constraints on the open cluster NGC 2477 using oscillating stars identified with TESS FFI
• Numerical Tests of Rotational Mixing in Massive Stars with the new Population Synthesis Code BONNFIRES
• Probing the physics of newly born magnetars through observation of superluminous supernovae
• Evolutionary process of the interacting binary V495 Centauri
• Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
• The impact of magnetic fields on momentum transport and saturation of shear-flow instability by stable modes
• Modified Gravity and the Flux-weighted Gravity-Luminosity Relationship of Blue Supergiant Stars
• Accretion induced black hole spin up revised by numerical GR MHD simulations
• Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations
• The sensitivity of presupernova neutrinos to stellar evolution models
• Effects of Rotationally-Induced Mixing in Compact Binary Systems with Low-Mass Secondaries and in Single Solar-Type Stars
• Supernovae from rotating stars
• Survival of the Fittest: Numerical Modeling of Supernova 2014C
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity
• Semi-Transparent Shear Turbulence in Hot Jupiter Atmospheres
• Long-term evolution of post-explosion Helium-star Companions of Type Iax Supernovae
• A Non-Detection of Red Supergiant Convection in Gaia
• Progenitor constraint with circumstellar material for the magnetar-hosting supernova remnant RCW 103
• Stellar age determination in the Mass-Luminosity Plane
• Massive stellar models: rotational evolution, metallicity effects
• A two-dimensional mixing length theory of convective transport
• The Masses Of The B-Stars In The High Galactic Latitude Eclipsing Binary IT Lib
• Rotating Supermassive Pop III Stars On The Main Sequence
• Exploring the relativistic regime with Newtonian hydrodynamics: II. An effective gravitational potential for rapid rotation
• Hydrogen-free Wolf-Rayet stars: Helium stars with envelope-inflation structure and rotation
• X-ray Flares Raising upon Magnetar Plateau as an Implication of a Surrounding Disk of Newborn Magnetized Neutron Star
• Magnetic quadri-dipolar stars rotating in vacuum
• Characterising the AGB bump and its potential to constrain mixing processes in stellar interiors
• Magnetic Webs in Stellar Radiative Zones
• Inner Engine Shutdown from Transitions in the Angular Momentum Distribution in Collapsars
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Rotational equilibria by Lagrangian variational principle: toward multi-dimensional stellar evolutions
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Nucleosynthesis in the accretion disks of Type II collapsars
• Effects of nucleon-nucleon short-range correlation and symmetry energy on the evolution of newly born magnetars
• Light elements in massive single and binary stars
• Spindown of massive main sequence stars in the Milky Way
• Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• Neutrino flavour as a test of the explosion mechanism of core-collapse supernovae
• Exploring the internal rotation of the extremely low-mass He-core white dwarf GD 278 with TESS asteroseismology
• Sodium enhancement in evolved cataclysmic variables
• Standing torsional Alfvén waves as the source of the rotational period variation in magnetic early-type stars
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• The efficiency of mixed modes for angular momentum transport
• A mixed helium-oxygen shell in some core-collapse supernova progenitors
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• Deciphering the period spacing pattern in the oscillation spectrum of the SPB star KIC 7760680
• The rotational shear in pre-collapse cores of massive stars
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• Fluorine abundances in CEMP stars at the lowest metallicity: Hints on the nature of the first stars
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Probing the models: Abundances for high-mass stars in binaries
• Effect of tides on the orbital evolution of the redback system PSR 1723-2837
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Proto-magnetar jets as central engines for broad-lined type Ic supernovae
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• The Blue supergiant problem and the main-sequence width
• The chemical evolution of the solar neighbourhood
• Between the cosmic-ray `knee' and the `ankle': Contribution from star clusters
• Jet-driven active galactic nucleus feedback in galaxy formation before black hole formation
• From Main Sequence Binary to Blast: MESA Modeling of the Double-Detonation Progenitor PTF1~J2238+7430
• Gravitational waves from magnetorotational core-collapse supernovae using 3D GRMHD simulations: effect of rotation and magnetic fields
• Simulations of Stellar Core Collapse, Bounce, and Postbounce Evolution with Boltzmann Neutrino Transport, and Implications for the Core Collapse Supernova Mechanism
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Non-LTE Equivalent Widths for NII with Error Estimates
• Modelling binary rotating stars by new population synthesis code BONNFIRES
• Insights from Asteroseismology of Massive Stars: The Need for Additional Angular Momentum Transport Mechanisms
• Spectrum of Global Magnetorotational Instability in a Narrow Transition Layer
• Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars
• The influence of rotation and metallicity on the explodability of massive stars
• Are There Pre-Main-Sequence/Black Hole X-ray Binaries?
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• A database of spectral energy distributions of progenitors of core-collapse supernovae
• Apsidal motion and proximity effects in the massive binary BD+60 497
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• Quantifying Systematic Age Discrepancies in Very Young Star Clusters
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
• Accretion in massive colliding wind binaries and the effect of wind momentum ratio
• Evolution and chemical and dynamical effects of high-mass stars