Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

Abstract

We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence stars. We provide three grids with different initial compositions tailored to compare with early OB stars in the Small and Large Magellanic Clouds and in the Galaxy. Each grid covers masses ranging from 5 to 60 Msun and initial rotation rates between 0 and about 600 km/s. To calibrate our models we used the results of the VLT-FLAMES Survey of Massive Stars. We determine the amount of convective overshooting by using the observed drop in rotation rates for stars with surface gravities log g < 3.2 to determine the width of the main sequence. We calibrate the efficiency of rotationally induced mixing using the nitrogen abundance determinations for B stars in the Large Magellanic cloud. We describe and provide evolutionary tracks and the evolution of the central and surface abundances. In particular, we discuss the occurrence of quasi-chemically homogeneous evolution, i.e. the severe effects of efficient mixing of the stellar interior found for the most massive fast rotators. We provide a detailed set of isochrones for rotating stars. Rotation as an initial parameter leads to a degeneracy between the age and the mass of massive main sequence stars if determined from its observed location in the Hertzsprung-Russell diagram. We show that the consideration of surface abundances can resolve this degeneracy.

Accepted for publication in A&A

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• Bow shocks, bow waves, and dust waves. I. Strong coupling limit
• Multiplicity of the red supergiant population in the young massive cluster NGC 330
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Three-dimensional Hydrodynamics Simulations of Precollapse Shell Burning in the Si- and O-rich Layers
• Testing the fossil field hypothesis: could strongly magnetised OB stars produce all known magnetars?
• How common is LBV S Dor variability at low metallicity?
• A VLT/FLAMES survey for massive binaries in Westerlund 1: VII. Cluster census
• B field in OB stars (BOB): The outstandingly strong magnetic field in the evolved He-strong star CPD-62 2124
• Superadiabaticity and the metallicity independence of the Humphreys-Davidson limit
• An absence of binary companions to Wolf-Rayet stars in the Small Magellanic Cloud: implications for mass loss and black hole masses at low metallicity
• Mass-loss rates of Very Massive Stars
• OB stars at the lowest Local Group metallicity: GTC-OSIRIS observations of Sextans A
• A detailed non-LTE analysis of LB-1: Revised parameters and surface abundances
• Gaia and HST astrometry of the very massive $\sim$150 $M_{\odot }$ candidate runaway star VFTS682
• Hubble Tarantula Treasury Project V. The star cluster Hodge 301: the old face of 30 Doradus
• Physical properties of the first spectroscopically confirmed red supergiant stars in the Sculptor Group galaxy NGC 55
• Diagnostic of the unstable envelopes of Wolf-Rayet stars
• Rotational Mixing in Be Stars: Nitrogen Abundances for a Sample of Be Stars from the MiMeS Survey
• The two components of the evolved massive binary LZ Cep. Testing the effects of binarity on stellar evolution
• The B-type Binaries Characterisation Programme II. VFTS 291: A stripped star from a recent mass transfer phase
• The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
• Modified Gravity and the Black Hole Mass Gap
• Phase-dependent study of near-infrared disk emission lines in LB-1
• The IACOB project IX. Building a modern empirical database of Galactic O9-B9 supergiants: sample selection, description, and completeness
• Age Dating Stellar Populations in the Near Infrared: An absolute age indicator from the presence/absence of red supergiants
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
• The IACOB project X. Large-scale quantitative spectroscopic analysis of Galactic luminous blue stars
• The flux-weighted gravity-luminosity relationship of blue supergiant stars as a constraint for stellar evolution
• Quantitative spectroscopy of B-type supergiants
• The magneto-rotational instability in massive stars
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• Extreme isolation of WN3/O3 stars and implications for their evolutionary origin as the elusive stripped binaries
• Role of supergiants in the formation of globular clusters
• A Strict Test of Stellar Evolution Models: The Absolute Dimensions of Massive Benchmark Eclipsing Binary V578 Mon
• Evidence of the Evolved Nature of the B[e] Star MWC 137
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• Calibrating the updated overshoot mixing model on eclipsing binary stars: HY Vir, YZ Cas, X2 Hya & VV Crv
• X-Shooting ULLYSES: Massive Stars at low metallicity VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• Sejong Open Cluster Survey (SOS). III. The Young Open Cluster NGC 1893 in the H II Region W8
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• Modeling overcontact binaries, I. The effect of tidal deformation
• 3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
• Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
• Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
• A new reference catalogue for the very metal-poor Universe: +150 OB stars in Sextans A
• The role of stellar expansion on the formation of gravitational wave sources
• Modeling contact binaries, II. The effect of energy transfer
• Chemical abundances of fast-rotating massive stars. II. Interpretation and comparison with evolutionary models
• On the stability of bow shocks generated by red supergiants: the case of IRC-10414
• The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints
• Inferring the parallax of Westerlund 1 from Gaia DR2
• A modern study of HD166734: a massive supergiant system
• Wind properties of Milky Way and SMC massive stars: empirical Z dependence from CMFGEN models
• A census of OBe stars in nearby metal-poor dwarf galaxies reveals a high fraction of extreme rotators
• A new and unusual LBV-like outburst from a Wolf-Rayet star in the outskirts of M33
• Influence of Rotation on Stellar Evolution
• Exploring the borderline between stable mass transfer and mergers in close binary evolution
• Spectroscopic patch model for massive stars using PHOEBE II and FASTWIND
• Spectroscopic evolution of massive stars near the main sequence at low metallicity
• The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars
• The VLT-FLAMES Tarantula Survey XXVII. Physical parameters of B-type main-sequence binary systems in the Tarantula nebula
• Accreting pre-main sequence models and abundance anomalies in globular clusters
• Towards a unified model of stellar rotation II: Model-dependent characteristics of stellar populations
• Evolution of massive stars with new hydrodynamic wind models
• X-Shooting ULLYSES: Massive Stars at low metallicity IX: Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• A rare early-type star revealed in the Wing of the Small Magellanic Cloud
• Confirming NGC 6231 as the parent cluster of the runaway high-mass X-ray binary HD 153919/4U 1700-37 with Gaia DR2
• Quantitative Spectroscopy of Supergiants in the Local Group Dwarf Galaxy IC 1613: Metallicity and Distance
• Classical Oe Stars in the Field of the Small Magellanic Cloud
• Metallicity dependence of turbulent pressure and macroturbulence in stellar envelopes
• A systematic study of super-Eddington layers in the envelopes of massive stars
• The VLT-FLAMES Tarantula Survey V. The peculiar B[e]-like supergiant, VFTS698, in 30 Doradus
• On the origin of close massive binaries in the M17 star-forming region
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• The blue supergiant MN18 and its bipolar circumstellar nebula
• Pulsational pair-instability and the mass gap of Population III Black Holes: Effects of overshooting
• Comment on "An excess of massive stars in the local 30 Doradus starburst"
• The distance, rotation, and physical parameters of zeta Pup
• Multiplicity among the cool supergiants in the Magellanic Clouds
• Empirical properties of Very Massive Stars
• The IACOB project XI. No increase of mass-loss rates over the bistability region
• The slowly pulsating B-star 18 Peg: A testbed for upper main sequence stellar evolution
• Orbital Parameters for the $250M_{\odot }$ Eta Carinae Binary System
• Optical spectroscopy of the blue supergiant Sk-69 279 and its circumstellar shell with SALT
• Characterization of the variability in the O+B eclipsing binary HD 165246
• TYC 3159-6-1: a runaway blue supergiant
• The VLT-FLAMES survey of massive stars: NGC346-013 as a test case for massive close binary evolution
• The Origin of B-Type Runaway Stars: Non-LTE Abundances as a Diagnostic
• Sejong Open Cluster Survey (SOS) - IV. The Young Open Clusters NGC 1624 and NGC 1931
• Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
• Constraints on the Compact Object Mass in the Eclipsing HMXB XMMU J013236.7+303228 in M33
• Exploring the stellar rotation of early-type stars in the LAMOST Medium-Resolution Survey. I. Catalog
• The Polstar High Resolution Spectropolarimetry MIDEX Mission
• The "Red Radio Ring": Ionised and Molecular Gas in a Starburst/Active Galactic Nucleus at $z\sim 2.55$
• On the bipolarity of Wolf-Rayet nebulae
• X-Shooting ULLYSES: Massive stars at low metallicity. IV. Spectral analysis methods and exemplary results for O stars
• The binary merger channel for the progenitor of the fastest rotating O-type star VFTS102
• Lithium and oxygen in globular cluster dwarfs and the early disc accretion scenario
• Dissecting the microphysics behind the metallicity-dependence of massive stars radii
• Astrophysical parameters and orbital solution of the peculiar X-ray transient IGR J00370+6122
• Induced differential rotation and mixing in asynchronous binary stars
• 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
• The Structure of the Young Star Cluster NGC 6231. I. Stellar Population
• Constraints on the Progenitor System of SN 2016gkg from a Comprehensive Statistical Analysis
• Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes
• Empirical mass-loss rates and clumping properties of O-type stars in the LMC
• Gaia TGAS search for Large Magellanic Cloud runaway supergiant stars:Candidate hypervelocity star discovery, and the nature of R71
• Melnick 33Na: a very massive colliding wind binary system in 30 Doradus
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• A strong neutron burst in jet-like supernovae of spinstars
• A VLT/FLAMES survey for massive binaries in Westerlund 1 V. the X-ray selected blue stragglers Wd1-27 and -30a
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• HD 152246 - a new high-mass triple system and its basic properties
• Physical parameters of red supergiants in dwarf irregular galaxies in the Local Group
• Lithium in coalesced non-compact stars
• The VLT-FLAMES Tarantula survey XX. The nature of the X-ray bright emission line star VFTS 399
• Mapping the core of the Tarantula Nebula with VLT-MUSE II. The spectroscopic Hertzsprung-Russell diagram of OB stars in NGC 2070
• A Study of Wolf-Rayet stars Formed via Chemically Homogeneous Evolution
• Comprehensive UV and Optical spectral analysis of Cygnus X-1: Stellar and wind parameters, abundances, and evolutionary implications
• A hydrodynamic study of the circumstellar envelope of alpha Scorpii
• Mixing of materials in magnetised core-collapse supernova remnants
• Can very massive Population III stars produce a super-collapsar?
• Supergiants and their shells in young globular clusters
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations
• A new outburst of the yellow hypergiant star Rho Cas
• A modern guide to quantitative spectroscopy of massive OB stars
• Extended supernova shock breakout signals from inflated stellar envelopes
• Can GW231123 have a stellar origin?
• The Impact of metallicity evolution of the universe on the maximum mass of LIGO binary black holes
• Production of secondary particles in heavy nuclei interactions in supernova remnants
• Revealing the Asymmetry of the Wind of the Variable Wolf-Rayet Star WR1 (HD4004) Through Spectropolarization
• V363 Cas: a new lithium rich Galactic Cepheid
• The mass distribution of stars stripped in binaries: The effect of metallicity
• Multiples among B stars in the Scorpius-Centaurus association
• Rotationally modulated variability and pulsations of the He-rich star CPD -62 2124 with an extraordinarily strong magnetic field
• Resolving the dynamical mass tension of the massive binary 9 Sagittarii
• Evolution of rotating massive stars with new hydrodynamic wind models
• Light or heavy supermassive black hole seeds: the role of internal rotation in the fate of supermassive stars
• Bayesian isochrone fitting and stellar ages
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• X-ray emission from star cluster winds in starburst galaxies
• PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03
• Stellar models of Betelgeuse constrained using observed surface conditions
• The multiplicity of massive stars in the Scorpius OB1 association through high-contrast imaging
• Observational implications of cosmologically coupled black holes
• The red supergiant population in the Perseus arm
• Cold gas in hot star clusters: the wind from the red supergiant W26 in Westerlund 1
• The VLT-FLAMES Tarantula Survey. XXIII: two massive double-lined binaries in 30~Doradus
• Discovery of a young and massive stellar cluster: Spectrophotometric near-infrared study of Masgomas-1
• Nitrogen chronology of massive main sequence stars
• Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
• Gaia BH1 and BH2 -- evolutionary models with overshooting of the black hole progenitors within the present-day binary separation
• Signatures of Rapidly Rotating Stars with Chemically Homogeneous Evolution in the First Galaxies
• A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
• The Maximum Black Hole Mass at Solar Metallicity
• Improving 1D stellar atmosphere models with insights from multi-dimensional simulations I. 1D vs 2D stratifications and spectral comparison for O stars
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• Populations of evolved massive binary stars in the Small Magellanic Cloud II: Predictions from rapid binary evolution
• An Apparent Precessing Helical Outflow from a Massive Evolved Star: Evidence for Binary Interaction
• Properties of luminous red supergiant stars in the Magellanic Clouds
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Non-synchronous rotations in massive binary systems. HD93343 revisited
• HD344787: a true Polaris analogue?
• The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction
• Period change and stellar evolution of $\beta$ Cephei stars
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• Rotational mixing in carbon-enhanced metal-poor stars with s-process enrichment
• Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• 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
• Rotational Variation Allows for Narrow Age Spread in the Extended Main Sequence Turnoff of Massive Cluster NGC 1846
• The canonical Luminous Blue Variable AG Car and its neighbor Hen 3-519 are much closer than previously assumed
• BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary
• The extreme O-type spectroscopic binary HD 93129A
• Extreme mass ratios and fast rotation in three massive binaries
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• pySTARBURST99: The Next Generation of STARBURST99
• Effects of the core-collapse supernova ejecta impact on a rapidly rotating massive companion star
• CPD-64 2731: a massive spun-up and rejuvenated high-velocity runaway star
• Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A
• BRITE photometry of the massive post-RLOF system HD149404
• A model of anisotropic winds from rotating stars for evolutionary calculations
• Towards early-type eclipsing binaries as extragalactic milestones: I. Physical parameters of OGLE-LMC-ECL-22270 and OGLE-LMC-ECL-06782
• An interferometric study of B star multiplicity
• He abundance of Dense Circumstellar Clumps in the Cassiopeia A Supernova Remnant
• The Transformative Journey of HD 93521
• Analytic approximations for massive close post-mass transfer binary systems
• Probing the low-mass end of the companion mass function for O-type stars
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
• The IACOB project XIV. New clues on the location of the TAMS in the massive star domain
• Surface chemical composition of single WNh stars
• Detection of single-degenerate massive binaries with Gaia: The impact of blue supergiants, triples, mass precision, and high-precision parallax requirements
• Massive pre-main-sequence stars in M17 -- Modelling hydrogen and dust in MYSO disks
• The VLT-FLAMES Tarantula Survey XXXII. Low-luminosity late O-type stars -- classification, main physical parameters, and silicon abundances
• Effects of Rotationally-Induced Mixing in Compact Binary Systems with Low-Mass Secondaries and in Single Solar-Type Stars
• Numerical Tests of Rotational Mixing in Massive Stars with the new Population Synthesis Code BONNFIRES
• The massive eclipsing system ALS 1135 and variable stars in the field of the distant OB association Bochum 7
• Enhanced mass-loss rate evolution of stars with $\gtrsim 18M_{\odot }$ and missing optically-observed type II core-collapse supernovae
• Broad Balmer Wings in BA Hyper/Supergiants Distorted by Diffuse Interstellar Bands: Five Examples in the 30 Doradus Region from the VLT-FLAMES Tarantula Survey
• Near-Infrared spectroscopy of the super star cluster in NGC1705
• Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
• X-Shooting ULLYSES: Massive Stars at Low Metallicity: XI. Pipeline-determined Physical Properties of Magellanic Cloud OB Stars
• Low energy core collapse supernovae in the frame of the jittering jets explosion mechanism
• Ultraviolet Spectropolarimetric Diagnostics of Hot Star Magnetospheres
• Stellar age determination in the Mass-Luminosity Plane
• Multiwavelength study of the fast rotating supergiant high-mass X-ray binary IGR J16465-4507
• X-Shooting ULLYSES: massive stars at low metallicity: XII. The clumped winds of O-type (super)giants in the Large Magellanic Cloud
• Rotating Supermassive Pop III Stars On The Main Sequence
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• The initial mass-remnant mass relation for core collapse supernovae
• Impact of rotation on stellar models
• Overshooting in the core helium burning stage of a $30M_{\odot }$ star using the $k$-$\omega$ model
• Wind and nebula of the M33 variable GR290 (WR/LBV)
• Detection of magnetic field in the B2 star $\rho$ Oph A with ESO FORS2
• A binary origin for the first isolated stellar-mass black hole detected with astrometric microlensing
• Surface abundances of OC supergiants
• LAMOST J040643.69+542347.8: the fastest Rotator in the Galaxy
• Magnetic Webs in Stellar Radiative Zones
• Masgomas-4: Physical characterization of a double-core obscured cluster with a massive and very young stellar population
• Hydrogen-free Wolf-Rayet stars: Helium stars with envelope-inflation structure and rotation
• Massive stars, successes and challenges
• News from Gaia on sigma Ori E: a case study for the wind magnetic braking process
• UV spectroscopy of the blue supergiant SBW1: the remarkably weak wind of a SN 1987A analog
• Extinction towards the cluster R136 in the Large Magellanic Cloud: An extinction law from the near-infrared to the ultraviolet
• The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium
• Moving inhomogeneous envelopes of stars
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Understanding the rotational variability of K2 targets. HgMn star KIC 250152017 and blue horizontal branch star KIC 249660366
• Spindown of massive main sequence stars in the Milky Way
• The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor
• Low-metallicity massive single stars with rotation. III. Source of ionization and C-IV emission in I Zw 18
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Binarity at LOw Metallicity (BLOeM): Projected rotational velocities
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• Characterization of the Most Luminous Star in M33: A Super Symbiotic Binary
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• New insight into the massive eccentric binary HD 165052: self-consistent orbital solution, apsidal motion, and fundamental parameters
• Looking for nebular He II emission south of the multiple-massive star system, HD 5980
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• Weighing stars from birth to death: mass determination methods across the HRD
• Evolutionary status of the Of?p star HD148937 and of its surrounding nebula NGC6164/5
• Gaia-ESO Survey: massive stars in the Carina Nebula. II. The spectroscopic analysis of the O-star population
• Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum
• Searching for compact objects in the single-lined spectroscopic binaries of the young Galactic cluster NGC 6231
• X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
• The population of Galactic supernova remnants in the TeV range
• Massive stars dying alone: the remote environment of SN 2010jp and its associated late-time source
• Formation of millisecond pulsar-helium star binaries
• Two New Rapidly-Rotating ON Stars Found With LAMOST
• X-Shooting ULLYSES: Massive stars at low metallicity. XIII. Putting the bi-stability jump to the test in the LMC
• Strong Variability in AzV 493, an Extreme Oe-Type Star in the SMC
• The Puzzling Spectrum of HD 94509
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• NGC 663 as a laboratory for massive star evolution
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• Rotational synchronisation of B-type binaries in 30 Doradus
• Two circumstellar nebulae discovered with the Wide-field Infrared Survey Explorer and their massive central stars
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling
• Luminous, rapidly declining supernovae as stripped transitional objects in low metallicity environments: the case of SN 2022lxg
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• The nature of the Cygnus extreme B-supergiant 2MASS J20395358+4222505
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• A near-UV reconnaissance of metal-poor massive stars
• Probing the models: Abundances for high-mass stars in binaries
• The NGC 346 massive star census: Nitrogen abundances for apparently single, narrow lined, hydrogen core burning B-type stars
• Stellar response after stripping as a model for common-envelope outcomes
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• The Blue supergiant problem and the main-sequence width
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
• Non-LTE Equivalent Widths for NII with Error Estimates
• Mass fluxes for O-type supergiants with metallicity Z = Z_{\sun}/5
• Light Axion Emission and the Formation of Merging Binary Black Holes
• An Alternative Formation Scenario for Uranium-rich Giants: Engulfing a Earth-like Planet
• A stringent upper limit on Be star fractions produced by binary interaction
• The wind properties of O-type stars at sub-SMC metallicity
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• The Predicted Properties of Helium-Enriched Globular Cluster Progenitors at High Redshift
• WR 63: A multiple system (O+O)+WR ?
• Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic technique
• Variability of Galactic blue supergiants observed with TESS
• Micro-turbulence across the Hertzsprung-Russell diagram. Observational constrains for stars in the MW
• X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
• The influence of rotation and metallicity on the explodability of massive stars
• SILCC -- IX. The multi-phase interstellar medium at low metallicity
• Blue Loops, Cepheids, and Forays into Axions
• The VLT-FLAMES survey of massive stars. NGC2004#115: A triple system hosting a possible short period B+BH binary
• SALT spectroscopy of the HMXB associated with the LMC supernova remnant MCSNR\,J0513$-$6724
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• The OVz stars in NGC 346: distribution, stellar parameters and insights into low-metallicity effects
• A magnetic field detection in the massive O-type bright giant 63 Oph
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• The Age of the R127 & R128 Clusters: Implications for the LBV
• Axion Instability Supernovae
• One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations
• Convective Penetration in Early-Type Stars
• The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812
• The incidence of LBV variability in the LMC
• Massive star evolution revealed in the Mass-Luminosity plane
• Spectroscopic Line Modeling of the Fastest Rotating O-type Stars
• 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