Mass-loss predictions for O and B stars as a function of metallicity

Abstract

We have calculated a grid of massive star wind models and mass-loss rates for a wide range of metal abundances between 1/100 and 10 Z/Zsun. The calculation of this grid completes the Vink et al. (2000) mass-loss recipe with an additional parameter Z. We have found that the exponent of the power law dependence of mass loss vs. metallicity is constant in the range between 1/30 and 3 Z/Zsun. The mass-loss rate scales as Mdot \propto Z^0.85 Vinf^p with p = -1.23 for stars with Teff \ga 25000 K, and p = -1.60 for the B supergiants with Teff \la 25000 K. Taking also into account the metallicity dependence of Vinf, using the power law dependence Vinf \propto Z^0.13 from Leitherer et al. (1992), the overall result of mass loss as a function of metallicity can be represented by Mdot \propto Z^0.69 for stars with Teff \ga 25000 K, and Mdot \propto Z^0.64 for B supergiants with Teff \la 25000 K. Our mass-loss predictions are successful in explaining the observed mass-loss rates for Galactic and Small Magellanic Cloud O-type stars, as well as in predicting the observed Galactic bi-stability jump. Hence, we believe that our predictions are reliable and suggest that our mass-loss recipe be used in future evolutionary calculations of massive stars at different metal abundance. A computer routine to calculate mass loss is publicly available.

Accepted by A&A, 16 pages, (email: [email protected])

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• The effect of 12C + 12C rate uncertainties on the evolution and nucleosynthesis of massive stars
• Driving classical Wolf-Rayet winds: A Γ- and Z-dependent mass-loss
• The formation of the extremely primitive star SDSS J102915+172927 relies on dust
• E-BOSS: An Extensive stellar BOw Shock Survey. II. Catalogue second release
• Numerical Simulations of Convective 3-Dimensional Red Supergiant Envelopes
• Predicting the Presence of Companions for Stripped-Envelope Supernovae: The Case of the Broad-Lined Type Ic SN 2002ap
• HR 5907: Discovery of the most rapidly rotating magnetic B-type star by the MiMeS Collaboration
• The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching and magnetic braking
• Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
• A JWST/NIRSpec Exploration of the Connection between Ionization Parameter, Electron Density, and Star-Formation-Rate Surface Density in z=2.7-6.3 Galaxies
• The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
• Type II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling
• Star formation efficiency as a function of metallicity: from star clusters to galaxies
• Massive star evolution : rotation, winds, and overshooting vectors in the Mass-Luminosity plane I. A calibrated grid of rotating single star models
• Triggering jet-driven explosions of core-collapse supernovae by accretion from convective regions
• Properties of WNh stars in the Small Magellanic Cloud: evidence for homogeneous evolution
• The ARAUCARIA project: Grid-Based Quantitative Spectroscopic Study of Massive Blue Stars in NGC55
• New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars. I. Method and first results
• JWST Imaging of Earendel, the Extremely Magnified Star at Redshift $z=6.2$
• Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity
• The Host Galaxies of Fast-Ejecta Core-Collapse Supernovae
• On the metallicity dependence of HMXBs
• Models for Massive Stellar Populations with Rotation
• Coalescing black hole binaries from globular clusters: mass distributions and comparison to gravitational wave data from GWTC-3
• Wind Roche lobe overflow in high mass X-ray binaries : a possible mass transfer mechanism for Ultraluminous X-ray sources
• Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system phi Persei
• Two bi-stability jumps in theoretical wind models for massive stars and the implications for Luminous Blue Variable supernovae
• A two-component model for fitting light-curves of core-collapse supernovae
• Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster
• Pair Instability Supernovae of Very Massive Population III Stars
• Discovery of a magnetic field in the rapidly-rotating O-type secondary of the colliding-wind binary HD 47129 (Plaskett's star)
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• Hierarchical black hole triples in young star clusters: impact of Kozai-Lidov resonance on mergers
• Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_{\odot }$ at a metallicity Z = 0.006
• The emergence of super-canonical stars in R136-type star-burst clusters
• Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
• The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems
• Very Massive Stars: a metallicity-dependent upper-mass limit, slow winds, and the self-enrichment of Globular Clusters
• The Early Phases of Supernova 2020pni: Shock-Ionization of the Nitrogen-Enriched Circumstellar Material
• Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution
• Fe emission and ionized excess absorption in the luminous quasar 3C109 with XMM-Newton
• The production of short-lived radionuclides by new non-rotating and rotating Wolf-Rayet model stars
• Dusty Wind-Blown Bubbles
• Progenitors of Type IIb Supernovae: I. Evolutionary Pathways and Rates
• MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars
• Stochasticity, a variable stellar upper-mass limit, binaries and star-formation rate indicators
• Multidimensional Simulations of Rotating Pair Instability Supernovae
• The Metallicity Dependence of the Minimum Mass for Core-Collapse Supernovae
• Using population synthesis of massive stars to study the interstellar medium near OB associations
• Internal entrainment and the origin of jet-related broad-band emission in Centaurus A
• Bonn Optimized Stellar Tracks (BoOST). Simulated Populations of Massive and Very Massive Stars for Astrophysical Applications
• Zooming in on Individual Star Formation: Low- and High-mass Stars
• Possible pair-instability supernovae at solar metallicity from magnetic stellar progenitors
• Wave-driven stellar expansion and binary interaction in pre-supernova outbursts
• Analytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure
• The thermonuclear production of F19 by Wolf-Rayet stars revisited
• A massive runaway star from 30 Doradus
• Black hole mergers in compact star clusters and massive black hole formation beyond the mass-gap
• GW190412 as a Third-Generation Black Hole Merger from a Super Star Cluster
• Coupling hydrodynamics with comoving frame radiative transfer: II. Stellar wind stratification in the high-mass X-ray binary Vela X-1
• Winds of low-metallicity OB-type stars: HST-COS spectroscopy in IC1613
• Photometric and Spectroscopic Studies of Massive Binaries in the Large Magellanic Cloud. I. Introduction and Orbits for Two Detached Systems: Evidence for a Mass Discrepancy?
• X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
• Common-Envelope Episodes that lead to Double Neutron Star formation
• The Formation of a 70 Msun Black Hole at High Metallicity
• Effects of anisotropic winds on massive stars evolution
• Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow
• Stellar and nebular diagnostics in the UV for star-forming galaxies
• The VLT-FLAMES Tarantula Survey XXVI: Properties of the O-dwarf population in 30 Doradus
• The Role of the Magnetorotational Instability in Massive Stars
• The Effect of Supernova Convection On Neutron Star and Black Hole Masses
• Accreting black hole binaries in globular clusters
• The Magnetic Early B-type Stars IV: Breakout or Leakage? H$\alpha$ emission as a diagnostic of plasma transport in centrifugal magnetospheres
• The effects of surface fossil magnetic fields on massive star evolution: II. Implementation of magnetic braking in MESA and implications for the evolution of surface rotation in OB stars
• Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type~II supernova progenitors
• Observational consequences of turbulent pressure in the envelopes of massive stars
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• Ultraviolet Detection of the Binary Companion to the Type IIb SN 2001ig
• Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity
• NGC 2770 - a supernova Ib factory?
• No breakdown of the radiatively-driven wind theory in low-metallicity environments
• An Infrared Nebula Associated with Delta Cephei: Evidence of Mass Loss?
• The VLT-FLAMES Tarantula Survey. XIII: On the nature of O Vz stars in 30 Doradus
• MOCCA Survey Database I: Dissolution of tidally filling star clusters harbouring BH subsystems
• On the Mass-Loss Rates of Massive Stars in the Low-Metallicity Galaxies IC 1613, WLM and NGC 3109
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- IV. cataclysmic variables -- properties of bright and faint populations
• Are some CEMP-s stars the daughters of spinstars?
• Line-driven ablation of circumstellar disks: I. Optically thin decretion disks of classical Oe/Be stars
• Radiation-driven winds of hot luminous stars. XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clusters
• A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the Main Sequence to planets
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Star Formation Regulation and Self-Pollution by Stellar Wind Feedback
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation III: dissecting black hole dynamics
• The winds of the hot massive first stars
• The VLT-FLAMES Tarantula Survey XXV. Surface nitrogen abundances of O-type giants and supergiants
• Modeling the early evolution of massive OB stars with an experimental wind routine
• Can Neutron-Star Mergers Explain the r-process Enrichment in Globular Clusters?
• Numerical Modeling of the Early Light Curves of Type IIP Supernovae
• Formation of wind-captured discs in Supergiant X-ray binaries : consequences for Vela X-1 and Cygnus X-1
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
• Radiative-transfer models for explosions from rotating and non-rotating single WC stars. Implications for SN1998bw and LGRB/SNe
• Understanding Compact Object Formation and Natal Kicks. IV. The case of IC 10 X-1
• Finding the First Cosmic Explosions II: Core-Collapse Supernovae
• Wolf-Rayet stars in the Small Magellanic Cloud as testbed for massive star evolution
• The HD5980 multiple system: Masses and evolutionary status
• Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• Binary population synthesis models for core-collapse gamma-ray burst progenitors
• Pulsations of red supergiant pair-instability supernova progenitors leading to extreme mass loss
• Modeling the near-infrared lines of O-type stars
• X-ray flares from the ultra-luminous X-ray source in NGC 5408
• Feedback regulated star formation: II. dual constraints on the SFE and the age spread of stars in massive clusters
• Population Synthesis of Black Hole Binaries with Normal-Star Companions: I. Detached Systems
• Variability of Red Supergiants in M31 from the Palomar Transient Factory
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• An Expanded HST/WFC3 Survey of M83: Project Overview and Targeted Supernova Remnant Search
• Ultraviolet spectra of extreme nearby star-forming regions: evidence for an overabundance of very massive stars
• On Rejuvenation in Massive Binary Systems
• X-ray emission from massive stars in Cyg OB2
• Supermassive Population III Supernovae and the Birth of the First Quasars
• Dependence of Convective Boundary Mixing on Boundary Properties and Turbulence Strength
• Can mass loss and overshooting prevent the excitation of g-modes in blue supergiants?
• SN 2017dio: a type-Ic supernova exploding in a hydrogen-rich circumstellar medium
• Grids of stellar models with rotation VII: Models from 0.8 to 300 M${}_{\odot }$ at super-solar metallicity (Z = 0.020)
• Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
• Rapidly evolving faint transients from stripped-envelope electron-capture supernovae
• Circumstellar interaction in supernovae in dense environments - an observational perspective
• The properties of ten O-type stars in the low-metallicity galaxies IC 1613, WLM and NGC 3109
• The Origin of inequality: isolated formation of a 30+10Msun binary black-hole merger
• A Spectroscopic Search for the non-nuclear Wolf-Rayet Population of the metal-rich spiral galaxy M83
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• The host galaxies of double compact objects merging in the local Universe
• Predicting Stellar-Mass Black Hole Populations in Globular Clusters
• Pre-collapse Properties of Superluminous Supernovae and Long Gamma-Ray Burst Progenitor Models
• Wind-envelope interaction as the origin of the slow cyclic brightness variations of luminous blue variables
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Mass loss and the Eddington parameter: a new mass-loss recipe for hot and massive stars
• Missing in Action: New Physics and the Black Hole Mass Gap
• Variability of Massive Stars with Known Spectral Types in the Small Magellanic Cloud Using 8 Years of OGLE-III Data
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
• Impact of Winds from Intermediate-Mass Stars on Molecular Cloud Structure and Turbulence
• How much hydrogen is in Type Ib and IIb supernova progenitors?
• Dust in the wind: the role of recent mass loss in long gamma-ray bursts
• Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
• Common envelope jets supernova (CEJSN) impostors resulting from a neutron star companion
• A trend in the effective spin distribution of LIGO binary black holes with mass
• Pair-Instability Supernovae via Collision Runaway in Young Dense Star Clusters
• Pair-Instability Supernova Simulations: Progenitor Evolution, Explosion, and Light Curves
• Spectroscopic evolution of massive stars on the main sequence
• The formation and coalescence sites of the first gravitational wave events
• NLTE models of line-driven stellar winds II. O stars in SMC
• Very Massive Stars and Pair-Instability Supernovae: Mass-loss Framework for low Metallicity
• Evidence for quasi-chemically homogeneous evolution of massive stars up to solar metallicity
• How runaway stars boost galactic outflows
• Fast & slow winds from supergiants and Luminous Blue Variables
• Terminal velocities of luminous, early-type SMC stars
• Population Synthesis of Black Hole X-Ray Binaries
• Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters
• Probing Star Formation at Low Metallicity: The Radio Emission of Super Star Clusters in SBS0335-052
• Stellar evolution of massive stars with a radiative alpha-omega dynamo
• Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
• Convective Properties of Rotating Two-Dimensional Core-Collapse Supernova Progenitors
• Angular momentum fluctuations in the convective helium shell of massive stars
• The evolution of planetary nebulae VII. Modelling planetary nebulae of distant stellar systems
• The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• Progenitors of early-time interacting supernovae
• Evolution of Wolf-Rayet stars as black hole progenitors
• Detection of magnetic fields in both B-type components of the $\epsilon$ Lupi system: a new constraint on the origin of fossil fields?
• Formation of supermassive black hole seeds in nuclear star clusters via gas accretion and runaway collisions
• An XMM-Newton observation of the massive binary HD159176
• Subsonic structure and optically thick winds from Wolf--Rayet stars
• Nucleosynthesis of binary-stripped stars
• Detecting stellar-wind bubbles through infrared arcs in HII regions
• Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• Massive Stars in the Galaxies of the Local Group
• The Star Formation History of the Milky Way's Nuclear Star Cluster
• Far-UV Spectroscopic Analyses of Four Central Stars of Planetary Nebulae
• Evolutionary models of red supergiants: Evidence for a metallicity-dependent mixing length and implications for Type IIP supernova progenitors
• Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia
• Host galaxies of SNe Ic-BL with and without long gamma-ray bursts
• Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
• Revisiting the explodability of single massive star progenitors of stripped-envelope supernovae
• Theoretical wind clumping predictions of OB supergiants from line-driven instability simulations across the bi-stability jump
• Presupernova neutrino events relating to the final evolution of massive stars
• Multiplicity of Galactic Luminous Blue Variable stars
• Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
• X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars
• Updating the theoretical tidal evolution constants: Apsidal motion and the moment of inertia
• A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes
• Characterizing Extreme Emission Line Galaxies II: A Self-Consistent Model of Their Ionizing Spectrum
• Spectroscopic evolution of very massive stars at Z = 1/2.5 Zsun
• Linear analyses for the stability of radial and nonradial oscillations of massive stars
• Modelling Luminous-Blue-Variable Isolation
• Illuminating the Primeval Universe with Type IIn Supernovae
• Nuclear timescale mass transfer in models of supergiant and ultra-luminous X-ray binaries
• A Population of Relic Intermediate-Mass Black Holes in the Halo of the Milky Way
• The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
• The MOSDEF Survey: The Metallicity Dependence of X-ray Binary Populations at $z\sim 2$
• Analysis of apsidal motion in eclipsing binaries using TESS data II. A test of internal stellar structure}
• SN 2020jfo: A short plateau Type II supernova from a low mass progenitor
• Effect of metallicity on the gravitational-wave signal from the cosmological population of compact binary coalescences
• On the nature of rapidly fading Type II supernovae
• Metallicity and the spectral energy distribution and spectral types of dwarf O-stars
• Zero and extremely low metallicity rotating massive stars: evolution, explosion, and nucleosynthesis up to the heaviest nuclei
• N-body models of globular clusters: metallicity, half-light radii and mass-to-light ratios
• Estimates for Lorentz factors of gamma-ray bursts from early optical afterglow observations
• Type II supernovae in low luminosity host galaxies
• How the breakout-limited mass in B-star centrifugal magnetospheres controls their circumstellar H-alpha emission
• Dynamical Tides Reexpressed
• Asteroseismological constraints on the coolest GW Vir variable star (PG 1159-type)PG 0122+200
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• Progenitor Model of SN 1987A Based on the Slow Merger Scenario
• Black hole spins in coalescing binary black holes
• The Star-Forming Region NGC 346 in the Small Magellanic Cloud with Hubble Space Telescope ACS Observations I. Photometry
• Integral Field Spectroscopy of Faint Haloes of Planetary Nebulae
• A Progenitor for the Extremely Luminous Type Ic Supernova 2007bi
• On the Formation of Galactic Black Hole Low-Mass X-ray Binaries
• Comparison of the optical light curves of hydrogen-rich and hydrogen-poor type II supernovae
• The Formation of Very Massive Stars
• The mass of the very massive binary WR21a
• Central Stars of Planetary Nebulae in the Large Magellanic Cloud: A Far-UV Spectroscopic Analysis
• Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties
• The massive binary CPD-41degr7742 II. Optical light curve and X-ray observations
• An explanation for the curious mass loss history of massive stars: from OB stars, through Luminous Blue Variables to Wolf-Rayet stars
• Exploring the GRB population: Robust afterglow modelling
• Evidence for the evolution of black hole mass function with redshift
• The theory of stellar winds
• A theoretical investigation of the Humphreys-Davidson limit at high and low metallicity
• Modeling Supermassive Primordial Stars with MESA
• Pair-Instability Supernovae in the Local Universe
• Stellar wind models of subluminous hot stars
• Towards a unified model of stellar rotation
• On the nature of the prototype LBV AG Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits
• The impact of stellar evolution on rotating star clusters: the gravothermal-gravogyro catastrophe and the formation of a bar of black holes
• Aluminium-26 from massive binary stars I: non-rotating models
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• Physical Properties of II Zw 40's Super Star Cluster and Nebula: New Insights and Puzzles from UV Spectroscopy
• Testing the predicted mass-loss bi-stability jump at radio wavelengths
• Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC346 in the SMC galaxy
• Supernovae within Pre-existing Wind-Blown Bubbles: Dust Injection vs. Ambient Dust Destruction
• Supernova Precursor Emission and the Origin of Pre-Explosion Stellar Mass-Loss
• Asteroseismology of the Nearby SN-II Progenitor Rigel Part II. ε-Mechanism Triggering Gravity-Mode Pulsations?
• Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae
• ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1 -- Determination of a new mass-loss rate prescription for red supergiants
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Mass loss of massive stars near the Eddington luminosity by core neutrino emission shortly before their explosion
• Radiation hydrodynamical simulations of eruptive mass Loss from progenitors of Type Ibn/IIn supernovae
• Mass discrepancy analysis for a select sample of Type II-Plateau supernovae
• X-ray photoionized bubble in the wind of Vela X-1 pulsar supergiant companion
• Explaining the differences in massive star models from various simulations
• Nonconservative Mass Transfer in Massive Binaries and the Formation of Wolf-Rayet+O Binaries
• Chemical composition of Galactic OB stars II. The fast rotator Z Oph
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• Evolution of massive stellar triples and implications for compact object binary formation
• Global hot-star wind models for stars from Magellanic Clouds
• The host galaxies of double compact objects across cosmic time
• Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud
• The cosmic carbon footprint of massive stars stripped in binary systems
• Wave-driven mass loss of stripped envelope massive stars: progenitor-dependence, mass ejection, and supernovae
• Comparing Spectral Models for ULXs with NGC 4517 ULX1
• Modeling broadband X-ray absorption of massive star winds
• The surface magnetic field and chemical abundance distributions of the B2V helium-strong star HD184927
• Constraining the Overcontact Phase in Massive Binary Evolution I. Mixing in V382 Cyg, VFTS 352, and OGLE SMC-SC10 108086
• HD 156324: a tidally locked magnetic triple spectroscopic binary with a disrupted magnetosphere
• Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au
• On the formation and evolution of the first Be star in a black hole binary MWC 656
• Physics and evolution of the most massive stars in 30 Dor. Mass loss, envelope inflation, and a variable upper stellar mass limit
• New mass-loss rates of B supergiants from global wind models
• WO-Type Wolf-Rayet Stars: the Last Hurrah of Massive Star Evolution
• Impact of metallicity on the evolution of young star clusters
• Roche-lobe overflow systems powered by black holes in young star clusters: the importance of dynamical exchanges
• Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
• GSH 138-01-94, an old supernova remnant in the far outer Galaxy
• On the Evolution of Supermassive Primordial Stars in Cosmological Flows
• A Galactic survey of radio jets from massive protostars
• A Study of Primordial Very Massive Star Evolution
• Fast Blue Optical Transients due to Circumstellar Interaction and the Mysterious Supernova SN 2018gep
• Multi-Epoch VLBA Observations of the Compact Wind-Collision Region in the Quadruple System Cyg OB2 #5
• Critical angular velocity and anisotropic mass loss of rotating stars with radiation-driven winds
• The impact of the FMR and starburst galaxies on the (low-metallicity) cosmic star formation history
• Evolution and CNO yields of Z=10^-5 stars and possible effects on CEMP production
• The Shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system
• Investigating the X-ray emission from the massive WR+O binary WR 22 using 3D hydrodynamical models
• On Monolithic Supermassive Stars
• The Host Galaxies of Long-Duration Gamma-Ray Bursts
• Infrared Photometric Properties of 709 Candidate Stellar Bowshock Nebulae
• Dynamically inflated wind models of classical Wolf-Rayet stars
• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
• Low-metallicity massive single stars with rotation. II. Predicting spectra and spectral classes of chemically-homogeneously evolving stars
• Is Betelgeuse the Outcome of a Past Merger?
• Ultraviolet Spectroscopy of Circumnuclear Star Clusters in M83
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• X-ray emission from BH+O star binaries expected to descend from the observed galactic WR+O binaries
• X-ray, UV and optical analysis of supergiants: $\epsilon$ Ori
• On the H$\alpha$ Behaviour of Blue Supergiants: Rise and Fall over the Bi-stability Jump
• A study of the effect of rotational mixing on massive stars evolution: surface abundances of Galactic O7-8 giant stars
• A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
• Upper Mass-Loss Limits and Clumping in the Intermediate and Outer Wind Regions of OB stars
• Massive black hole assembly in nuclear star clusters
• Black hole - black hole total merger mass and the origin of LIGO/Virgo sources
• Observational properties of massive black hole binary progenitors
• A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars
• NLTE models of line-driven stellar winds I. Method of calculation and first results for O stars
• Fast-rotating massive Population~III stars as possible sources of extreme N-enrichment in high-redshift galaxies
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• Emission-line Wings Driven by Lyman Continuum in the Green Pea Analog Mrk 71
• The p-process in exploding rotating massive stars
• The Binding Energy Parameter for Common Envelope Evolution
• Evidence for Very Massive Stars in extremely UV-bright star-forming galaxies at $z\sim 2.2-3.6$
• Evolutionary models of short-period soft X-ray transients: comparison with observations
• On the role of supernova kicks in the formation of Galactic double neutron star systems
• A peculiar Of star in the Local Group galaxy IC 1613
• Progenitors of Type IIb Supernovae: II. Observable Properties
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• On the Common Envelope Efficiency
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Population III Hypernovae
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• On the Red Supergiant Wind Kink. A Universal mass-loss concept for massive stars
• Magnetohydrodynamic simulations of mechanical stellar feedback in a sheet-like molecular cloud
• A new mechanical stellar wind feedback model for the Rosette Nebula
• The Tarantula Massive Binary Monitoring V. R 144: a wind-eclipsing binary with a total mass > 140 Msun
• Explaining the multiple populations in globular clusters by multiple episodes of star formation and enrichment without gas expulsion from massive star feedback
• GRB 160625B: Evidence for a Gaussian-Shaped Jet
• A variable ultra-luminous X-ray source in the colliding galaxy NGC 7714
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• An ALMA 3mm continuum census of Westerlund 1
• Stellar Core-Merger-Induced Collapse: New Formation Pathways for Black Holes, Thorne-$\dot{\mathrm{Z}}$ytkow objects, Magnetars and Superluminous Supernovae
• The fate of Cyg X-1: an empirical lower limit on BH-NS merger rate
• The impact of realistic red supergiant mass-loss on stellar evolution
• How common is LBV S Dor variability at low metallicity?
• Bow shocks, bow waves, and dust waves. I. Strong coupling limit
• Asymmetric core collapse of rapidly rotating massive star
• Constraining GRB progenitor models by probing Wolf-Rayet wind geometries in the Large Magellanic Cloud
• Investigating the origin of cyclical wind variability in hot, massive stars - I. On the dipolar magnetic field hypothesis
• The magnetic field and spectral variability of the He-weak star HR 2949
• Finding the First Cosmic Explosions. IV. 90 - 140 M${}_{\odot }$ Pair-Instability Supernovae
• Initial conditions for globular clusters and assembly of the old globular cluster population of the Milky Way
• Circum-stellar medium around rotating massive stars at solar metallicity
• Characterizing dynamical states of Galactic open clusters with Gaia DR2
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants
• On the origin of nitrogen at low metallicity
• The connection between merging double compact objects and the Ultraluminous X-ray Sources
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Stellar population of the superbubble N206 in the LMC I. Analysis of the Of-type stars
• Close binary evolution. III. Impact of tides, wind magnetic braking, and internal angular momentum transport
• Mass-loss predictions for evolved very metal-poor massive stars
• Evolution and final fate of massive post-common-envelope binaries
• OB stars at the lowest Local Group metallicity: GTC-OSIRIS observations of Sextans A
• Properties of six short-period massive binaries: a study of the effects of binarity on surface chemical abundances
• Probing the initial mass function of the first stars with transients
• Superadiabaticity and the metallicity independence of the Humphreys-Davidson limit
• Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods
• Clumping and X-Rays in cooler B supergiant stars
• CNO driven winds of hot first stars
• Mass-loss rates of Very Massive Stars
• A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae
• Exploring stellar evolution with gravitational-wave observations
• 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
• Winds in Star Clusters Drive Kolmogorov Turbulence
• The Evolution of Gamma-ray Burst Jet Opening Angle through Cosmic Time
• Constraining Compact Object Formation with 2M0521
• Close Encounters of Wide Binaries Induced by the Galactic Tide: Implications for Stellar Mergers and Gravitational-Wave Sources
• Black hole - neutron star mergers: The first mass gap and kilonovae
• Apsidal motion in the massive binary HD152218
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• Predictions of a simple parametric model of hierarchical black hole mergers
• Modified Gravity and the Black Hole Mass Gap
• Exploring compact binary populations with the Einstein Telescope
• The 2.35 year itch of Cyg OB2 #9. II. Radio monitoring
• The two components of the evolved massive binary LZ Cep. Testing the effects of binarity on stellar evolution
• The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
• Average opacity calculation for core-collapse supernovae
• A Spectroscopic Study of the Rich Supernova Remnant Population in M83
• A Chandra X-ray Study of NGC 1068: II. The Luminous X-ray Source Population
• A transdimensional Bayesian method to infer the star formation history of resolved stellar populations
• A VLT spectroscopic study of the ultracompact HII region G29.96-0.02
• Demographics of triple systems in dense star clusters
• Red Supergiants in M31: The Humphreys-Davidson limit at high metallicity
• Evolution of rotation in rapidly rotating early-type stars during the main sequence with 2D models
• Hydrodynamic simulations of mechanical stellar feedback in a molecular cloud formed by thermal instability
• The pulsating magnetosphere of the extremely slowly rotating magnetic $\beta$ Cep star ${\xi }^1$ CMa
• Evidence that Gamma-ray Burst 130702A Exploded in a Dwarf Satellite of a Massive Galaxy
• On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613
• What binary systems are the most likely sources for periodically repeating FRBs?
• The flux-weighted gravity-luminosity relationship of blue supergiant stars as a constraint for stellar evolution
• Extreme isolation of WN3/O3 stars and implications for their evolutionary origin as the elusive stripped binaries
• The Ofpe/WN9 stars in M33
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• A test for the theory of colliding winds: the periastron passage of 9 Sagittarii I. X-ray and optical spectroscopy
• Propulsion of Spacecrafts to Relativistic Speeds Using Natural Astrophysical Sources
• XMM-Newton view of the N 206 superbubble in the Large Magellanic Cloud
• The impact of metallicity-dependent mass loss versus dynamical heating on the early evolution of star clusters
• Population synthesis on high-mass X-ray binaries: prospects and constraints from the universal X-ray luminosity function
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• A Strict Test of Stellar Evolution Models: The Absolute Dimensions of Massive Benchmark Eclipsing Binary V578 Mon
• Integral Field Spectroscopy of Massive Young Stellar Objects in the N113 H\,{\sc ii} Region in the Large Magellanic Cloud
• In pursuit of gamma-ray burst progenitors: the identification of a sub-population of rotating Wolf-Rayet stars
• The Impact of Progenitor Mass Loss on the Dynamical and Spectral Evolution of Supernova Remnants
• The Ionizing Spectra of Extremely Metal-Poor O Stars: Constraints from the Only HII Region in Leo P
• The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• Very Massive Star Models: I. Impact of Rotation and Metallicity and Comparisons with Observations
• The effect of the centrifugal acceleration on period spacings of gravito-inertial modes in intermediate-mass stars
• The young stellar population of IC 1613. III. New O-type stars unveiled by GTC-OSIRIS
• Modeling overcontact binaries, I. The effect of tidal deformation
• Optical/near-infrared observations of the Fried Egg Nebula: Multiple shell ejections on a 100 yr timescale from a massive yellow hypergiant
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• Effect of mass loss due to stellar winds on the formation of supermassive black hole seeds in dense nuclear star clusters
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Formation and Evolution of Ultraluminous X-ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• X-Shooting ULLYSES: Massive Stars at low metallicity VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• On the reliability of CIV 1549 as an abundance indicator for high redshift star-forming galaxies
• The ionization structure of early-B supergiant winds
• The ultraviolet and optical spectra of luminous B-type stars in the Small Magellanic Cloud
• Confirming the oblique rotator model for the extremely slowly rotating O8f?p star HD 108
• Wind properties of Milky Way and SMC massive stars: empirical Z dependence from CMFGEN models
• The role of stellar expansion on the formation of gravitational wave sources
• The origin of circumstellar features in the spectra of hot DA white dwarfs
• Magnetic characterization of the SPB/$\beta$ Cep hybrid pulsator HD 43317
• Detecting strongly lensed supernovae at z ~ 5-7 with LSST
• A modern study of HD166734: a massive supergiant system
• 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
• Chemical abundances of fast-rotating massive stars. II. Interpretation and comparison with evolutionary models
• Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
• Finding Black Holes with Black Boxes -- Using Machine Learning to Identify Globular Clusters with Black Hole Subsystems
• Spectroscopic evolution of massive stars near the main sequence at low metallicity
• Revealing Efficient Dust-Formation at Low Metallicity in Extragalactic Carbon-Rich Wolf-Rayet Binaries
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• Demonstration of a novel method for measuring mass-loss rates for massive stars
• NU Ori: a hierarchical triple system with a strongly magnetic B-type star
• Evolutionary status of Polaris
• Dynamics of massive stellar black holes in young star clusters and the displacement of ultra-luminous X-ray sources
• Probing the weak wind phenomenon in Galactic O-type giants
• Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E
• Spectroscopic patch model for massive stars using PHOEBE II and FASTWIND
• Apsidal motion in the massive binary HD 152248 -- Constraining the internal structure of the stars
• New hydrodynamic solutions for line-driven winds of hot massive stars using Lambert $W$-function
• Discovery of X-ray emission from young suns in the Small Magellanic Cloud
• Modelling type IIP/IIL supernovae interacting with recent episodic mass ejections from their presupernova stars with MESA & SNEC
• The CO White Dwarf + Intermediate Mass/Massive Star Binary Evolution: Possible Merger Origins for Peculiar Type Ia and II Supernovae
• Applying the metallicity-dependent binary fraction to double white dwarf formation: Implications for LISA
• Star formation around the mid-infrared bubble CN 148
• Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star
• HD 164492C: a rapidly-rotating, H$\alpha$-bright, magnetic early B star associated with a 12.5d spectroscopic binary
• Evolution of massive stars with new hydrodynamic wind models
• UV diagnostic of porosity-free mass-loss estimates in B stars
• 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
• Formation and Destiny of White Dwarf and Be Star Binaries
• Towards a unified model of stellar rotation II: Model-dependent characteristics of stellar populations
• Shock-heated radiation-driven outflows as a solution to the weak-wind problem of late O-type stars
• Magnetism in High-Mass Stars
• The eclipsing binary systems with $\delta$ Scuti component. I. KIC 10661783
• Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method
• X-ray emission from the giant magnetosphere of the magnetic O-type star NGC 1624-2
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• Self-consistent solutions for line-driven winds of hot massive stars. The m-CAK procedure
• First detections of FS Canis Majoris stars in clusters. Evolutionary state as constrained by coeval massive stars
• A systematic study of super-Eddington layers in the envelopes of massive stars
• XMM-Newton observations of the giant HII region N11 in the LMC
• Mass loss and stellar superwinds
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• On the possibility of disk-fed formation in supergiant high-mass X-ray binaries
• Magnetic inhibition of convection in O star envelopes
• Centrifugally Driven Mass Loss and Outbursts of Massive Stars
• Gas-phase Fe/O and Fe/N abundances in Star-Forming Regions. Relations between nucleosynthesis, metallicity and dust
• Hydrodynamical models of cometary HII regions
• The Gaia-ESO Survey: The analysis of the hot-star spectra
• e-MERLIN 21cm constraints on the mass-loss rates of OB stars in Cyg OB2
• On the evolutionary state of massive stars in transition phases in M33
• Metallicity dependence of turbulent pressure and macroturbulence in stellar envelopes
• SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
• X-ray diagnostics of massive star winds
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• Impact of main-sequence mass loss on the appearance, structure and evolution of Wolf-Rayet stars
• Sensitivity of ${}^{44}$Ti and ${}^{56}$Ni production in CCSN shock-driven nucleosynthesis to reaction rates
• The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: spectroscopy, orbital analysis, formation, and evolution
• Improved velocity law parameterization for hot star winds
• A Population of Neutron Star Ultraluminous X-ray Sources with A Helium Star Companion
• The optical rebrightening of GRB100814A: an interplay of forward and reverse shocks?
• X-ray and optical spectroscopy of the massive young open cluster IC1805
• The IACOB project XI. No increase of mass-loss rates over the bistability region
• Stellar wind models of central stars of planetary nebulae
• Eruption of the Envelope of Massive Stars by Energy Injection with Finite Duration
• Red supergiants and stellar evolution
• Aluminium-26 from massive binary stars III. Binary stars up to core-collapse and their impact on the early Solar System
• CHIPS: Complete History of Interaction-Powered Supernovae
• Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
• Radio Supernovae in the Great Survey Era
• Red Supergiants, Yellow Hypergiants, and Post-RSG Evolution
• Optical spectroscopy of X-Mega targets in the Carina Nebula - V. The spectroscopic binary HD93161A and its visual companion HD93161B
• Wind-powered ultraluminous X-ray sources
• McFacts III: Compact binary mergers from AGN disks over an entire synthetic universe
• X-Shooting ULLYSES: Massive stars at low metallicity. IV. Spectral analysis methods and exemplary results for O stars
• Merging binary black holes formed through double-core evolution
• Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectors
• Binarity at Low Metallicity (BLOeM) -- Multiplicity properties of Oe and Be stars
• Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
• Pulsations as a Driver for LBV Variability
• New multiwavelength observations of the Of?p star CPD -28 2561
• Dissecting the microphysics behind the metallicity-dependence of massive stars radii
• Black Holes In Young Stellar Clusters
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• Method and new tabulations for flux-weighted line-opacity and radiation line-force in supersonic media
• 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
• Ultraviolet Line Profiles of Slowly Rotating Massive Star Winds Using the "Analytic Dynamical Magnetosphere" Formalism
• Collective Properties of X-ray Binary Populations of Galaxies. I. Luminosity and Orbital Period Distributions of High-Mass X-ray Binaries
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• Pre-explosion dynamo in the cores of massive stars
• LMC X-1: A New Spectral Analysis of the O-star in the binary and surrounding nebula
• Constraints on the Progenitor System of SN 2016gkg from a Comprehensive Statistical Analysis
• Influence of XUV radiation on Pv ionization fraction in hot star winds
• EDGE-INFERNO: Simulating every observable star in faint dwarf galaxies and their consequences for resolved-star photometric surveys
• The peculiar circumstellar environment of NGC2024-IRS2
• Empirical mass-loss rates and clumping properties of O-type stars in the LMC
• Catastrophic Cooling in Superwinds. III. Non-equilibrium Photoionization
• X-ray emission from hydrodynamical simulations in non-LTE wind models
• Progenitor mass constraints for the type Ib intermediate-luminosity SN 2015ap and the highly extinguished SN 2016bau
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• Exploring the Energy Sources Powering the Light Curve of the Type Ibn Supernova PS15dpn and the Mass-Loss History of the SN Progenitor
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• Comparison between the first and second mass eruptions from progenitors of Type IIn supernovae
• The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars
• Intermediate Luminosity Optical Transients (ILOTs) from merging giants
• Episodic modulations in supernova radio light curves from luminous blue variable supernova progenitor models
• The impact of convective criteria on the properties of massive stars
• Accretion mode of the Ultra-Luminous X-ray source M82 X-2
• Extended Red Objects and Stellar Wind Bow Shocks in the Carina Nebula
• An Observational Evaluation of Magnetic Confinement in the Winds of BA Supergiants
• Population synthesis of ultraluminous X-ray sources with magnetised neutron stars
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• Supergiants and their shells in young globular clusters
• Apsidal motion in massive eccentric binaries in NGC 6231: The case of HD 152219
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• Comprehensive UV and Optical spectral analysis of Cygnus X-1: Stellar and wind parameters, abundances, and evolutionary implications
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds
• Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2{\mathrm{Z}}_{\odot }$
• The jittering jets explosion mechanism (JJEM) in electron capture supernovae
• On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations
• Understanding the progenitor formation galaxies of merging binary black holes
• Theoretical wind clumping predictions from 2D LDI models of O-star winds at different metallicities
• Formation of periodic FRB in binary systems with eccentricity
• A wind-blown bubble in the Central Molecular Zone cloud G0.253+0.016
• MOBSTER -- V: Discovery of a magnetic companion star to the magnetic $\beta$ Cep pulsator HD 156424
• A Study of Wolf-Rayet stars Formed via Chemically Homogeneous Evolution
• The radial distribution of supernovae compared to star formation tracers
• First constraints on the magnetic field strength in extra-Galactic stars: FORS2 observations of Of?p stars in the Magellanic Clouds
• Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies
• O-star mass-loss rates at low metallicity
• Evolution and Nucleosynthesis of Very Massive Stars
• Pulsations in B-type supergiants with masses $M<20M_{\odot }$ before and after core helium ignition
• The Impact of metallicity evolution of the universe on the maximum mass of LIGO binary black holes
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Towards an understanding of long gamma-ray burst environments through circumstellar medium population synthesis predictions
• Evolution of rotating massive stars with new hydrodynamic wind models
• Impact of binary interaction on the evolution of blue supergiants
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Inferring CSM Properties of Type II SNe Using a Magnitude-Limited ZTF Sample
• The Trace of the CNO Cycle in the Ring Nebula NGC6888
• Pulsation-driven mass loss from massive stars behind stellar mergers in metal-poor dense clusters
• Detection of intrinsic variability in the eclipsing massive main sequence O+B binary HD 165246
• The MODEST questions: challenges and future directions in stellar cluster research
• Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
• Accretion disks in Algols: progenitors and evolution
• Modelling the photometric variability of magnetic massive stars with the Analytical Dynamical Magnetosphere model
• Simulating the Response of the Secondary Star of Eta Carinae to Mass Accretion at Periastron Passage
• Effects of axions on Population III stars
• X-rays from Hot Subdwarfs
• The hydrogen clock to infer the upper stellar mass
• Very massive star winds as sources of the short-lived radioactive isotope ${}^{26}$Al
• Titanium and Iron in the Cassiopeia A Supernova Remnant
• Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at SMC metallicity
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• The Evolution of Population III and Extremely Metal-Poor Binary Stars
• Hot subdwarf wind models with accurate abundances I. Hydrogen dominated stars HD 49798 and BD+18${}^{\circ }$2647
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Mass-loss rates for hot luminous stars: the influence of line branching
• A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
• An exceptional population of late-type WC stars in the metal-rich spiral galaxy
• The multiplicity of massive stars in the Scorpius OB1 association through high-contrast imaging
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• The Evolution of Accreting Population III Stars at 10${}^{-6}$-10${}^3$ M${}_{\odot }$/yr
• Mass loss rates from mid-IR excesses in LMC and SMC O stars
• Signatures of Rapidly Rotating Stars with Chemically Homogeneous Evolution in the First Galaxies
• NGC 6611 601: A hot pre-main sequence spectroscopic binary containing a centrifugal magnetosphere host star
• PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03
• Mid-Infrared diagnostics of metal-rich HII regions from VLT and Spitzer Spectroscopy of Young Massive Stars in W31
• The long and the short of it: modelling double neutron star and collapsar Galactic dynamics
• Deciphering stellar metallicities in the early Universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
• New self-consistent wind parameters fitting optical spectra of O-type stars observed with HERMES spectrograph
• Gaia BH1 and BH2 -- evolutionary models with overshooting of the black hole progenitors within the present-day binary separation
• Nitrogen chronology of massive main sequence stars
• Whispering in the dark: Faint X-ray emission from black holes with OB star companions
• Massive stars evolution with new C12+C12 nuclear reaction rate -- the core carbon-burning phase
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
• The impact of binaries on the evolution of star clusters from turbulent molecular clouds
• The Maximum Black Hole Mass at Solar Metallicity
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Improving 1D stellar atmosphere models with insights from multi-dimensional simulations I. 1D vs 2D stratifications and spectral comparison for O stars
• Stellar feedback impact on the ionized gas kinematics in the dwarf galaxy Sextans A
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• The magnetic field and magnetosphere of Plaskett's star: A fundamental shift in our understanding of the system
• Spitzer observations of Bow Shocks and Outflows in RCW 38
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
• Hot star wind models with new solar abundances
• Modeling non-thermal emission from stellar bow shocks
• First VLT/X-shooter spectroscopy of early-type stars outside the Local Group
• Simulations of the line-driven instability in magnetic hot star winds
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Great Balls of FIRE III: Modeling Black Hole Mergers from Massive Star Clusters in Simulations of Galaxies
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• The Temperature Structure of Be Star Disks in the Small Magellanic Cloud
• Effects of the core-collapse supernova ejecta impact on a rapidly rotating massive companion star
• 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
• pySTARBURST99: The Next Generation of STARBURST99
• The Extremely Metal-Poor SN 2023ufx: A Local Analog to High-Redshift Type II Supernovae
• 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
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
• Magnetic characterization and variability study of the magnetic SPB star o Lup
• Magnetic Braking at work in binaries
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• Surrogate forward models for population inference on compact binary mergers
• Magnetic field geometry and magnetospheric environment of the strongly magnetic Of?p star NGC 1624-2
• BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• Hunting gravitational wave black holes with microlensing
• Unveiling the nitrogen-rich massive star in the metal-poor galaxy NGC 4068
• Exploring the connection between atmosphere models and evolution models of very massive stars
• Magnetic Archaeology of Early-Type Stellar Dynamos
• Formation and fate of low metallicity stars in IllustrisTNG50
• Close encounters of black hole - star binaries with stellar-mass black holes
• The long-period massive binary HD~54662 revisited
• Galactic population of black holes in detached binaries with low-mass stripped helium stars: the case of LB-1 (LS~V+22~25)
• The Carina High-contrast Imaging Project for massive Stars (CHIPS): II. O stars in Trumpler~14
• Discovery of Magnetospheric Interactions in the Doubly-Magnetic Hot Binary $\epsilon$ Lupi
• Galactic Outflows and Evolution of the Interstellar Medium
• Strong nebular HeII emission induced by He${}^{+}$ ionizing photons escaping through the clumpy winds of massive stars
• Probing the low-mass end of the companion mass function for O-type stars
• Dense molecular globulettes and the dust arc towards the runaway O star AE Aur (HD 34078)
• Spin evolution of neutron stars in wind-fed high mass X-ray binaries
• A model of anisotropic winds from rotating stars for evolutionary calculations
• Evolution of Rotating 25 M${}_{\odot }$ Population III star: Physical Properties and Resulting Supernovae
• High-Mass X-Ray Binaries with Be Donors as Ultraluminous X-Ray Sources
• B stars seen at high resolution by XMM-Newton
• Enhanced mass-loss rate evolution of stars with $\gtrsim 18M_{\odot }$ and missing optically-observed type II core-collapse supernovae
• Applications of Stellar Population Synthesis in the Distant Universe
• FS CMa type binaries
• Creating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra
• Modified Gravity and the Flux-weighted Gravity-Luminosity Relationship of Blue Supergiant Stars
• The Origin of the Possible Massive Black Hole in the Progenitor System of iPTF13bvn
• Common Envelope Mechanisms: Constraints from the X-ray Luminosity Function of High Mass X-ray Binaries
• On the Anti-Correlation between Duration and Redshift in Gamma-ray Bursts
• Isotopic ratios for C, N, Si, Al, and Ti in C-rich presolar grains from massive stars
• Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
• Metal-enriched Pair-instability supernovae: Effects of rotation
• Surface chemical composition of single WNh stars
• X-Shooting ULLYSES: Massive Stars at Low Metallicity: XI. Pipeline-determined Physical Properties of Magellanic Cloud OB Stars
• Blue luminous stars in nearby galaxies - UIT005: a possible link to the luminous blue variable stage
• Numerical Tests of Rotational Mixing in Massive Stars with the new Population Synthesis Code BONNFIRES
• Very Large Array and Jansky Very Large Array observations of the compact radio sources in M8
• Constraining the fundamental parameters of the O-type binary CPD-41degr7733
• Stellar-wind feedback and magnetic fields around young compact star clusters: 3D MHD simulations
• 26Al and 60Fe from massive stars
• Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
• Nucleosynthesis from massive stars 50 years after B2FH
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• X-Shooting ULLYSES: massive stars at low metallicity: XII. The clumped winds of O-type (super)giants in the Large Magellanic Cloud
• Statistics of Magrathea exoplanets beyond the Main Sequence. Simulating the long-term evolution of circumbinary giant planets with TRES
• The First Candidate Colliding-Wind Binary in M33
• Mechanisms for high spin in black-hole neutron-star binaries and kilonova emission: inheritance and accretion
• UV Spectropolarimetry with Polstar: Massive Star Binary Colliding Winds
• Non-linear Three-mode Coupling of Gravity Modes in Rotating Slowly Pulsating B Stars: Stationary Solutions and Modeling Potential
• Dust Grain Growth & Dusty Supernovae in Low-Metallicity Molecular Clouds
• Low energy core collapse supernovae in the frame of the jittering jets explosion mechanism
• Formation rate of LB-1-like systems through dynamical interactions
• Instability of LBV-stars against radial oscillations
• Spectroscopic study of the optical counterpart to the Fast X-ray Transient IGR J17544-2619 based on observations at the 1.5-m RTT-150 telescope
• Ongoing star formation in the proto-cluster IRAS 22134+5834
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• A binary origin for the first isolated stellar-mass black hole detected with astrometric microlensing
• The initial mass-remnant mass relation for core collapse supernovae
• Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
• Electron Scattering Emission in the Light Curves of Stars with Centrifugal Magnetospheres
• Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
• Probing gamma-ray bursts observed at very high energies through their afterglow
• Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity
• Effect of rotational mixing and metallicity on the hot star wind mass-loss rates
• The fate of rotating massive stars across cosmic times
• Stellar age determination in the Mass-Luminosity Plane
• Binary imposters: Mergers in massive hierarchical triple stars
• Type IIP Supernova Progenitors II: Stellar Mass and Obscuration by the Dust in the Circumstellar Medium
• Moving inhomogeneous envelopes of stars
• Variable millimetre radiation from the colliding-wind binary Cyg OB2 #8A
• Shadows of the Colossus: Hierarchical Black Hole Mergers in a 10-million-body Globular Cluster Simulation
• Very massive stars at low metallicity: evolution, synthetic spectroscopy, and impact on the integrated light of starbursts
• Black hole mass function shift in proto-stellar-clusters driven by gas accretion
• On the mass-function of GWTC-2 binary black hole systems and their progenitors
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• An Exploration of X-ray Supernova Remnants in the Milky Way and Nearby Galaxies
• A new long gamma-ray burst formation pathway at solar metallicity
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• NLTE wind models of hot subdwarf stars
• Inner and outer star forming regions over the disks of spiral galaxies. II. A comparative of physical properties and evolutionary stages
• Monte Carlo Radiation Transport for Astrophysical Transients Powered by Circumstellar Interaction
• Ultraviolet Spectropolarimetry With Polstar: Using Polstar to test Magnetospheric Mass-loss Quenching
• UV spectroscopy of the blue supergiant SBW1: the remarkably weak wind of a SN 1987A analog
• Modelling multiwavelength emission of Ultra-luminous X-ray Sources accreting above the Eddington limit
• X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
• Far-infrared emission of massive stars
• Heavy element contributions of rotating massive stars to Interstellar Medium
• The neutrino emission from thermal processes in very massive stars in the local universe
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. III. Evolution
• Investigating episodic mass loss in evolved massive stars: III. Spectroscopy of dusty massive stars in three northern galaxies
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant
• Dark Matter Mini-halo around the Compact Objects: the Formation, Evolution and Possible Contribution to the Cosmic Ray Electrons/Positrons
• Spindown of massive main sequence stars in the Milky Way
• Blue Supergiant X-ray Binaries in the Nearby Dwarf Galaxy IC 10
• Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes
• Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum
• VLT/MUSE and ATCA observations of the host galaxy of the short GRB 080905A at z=0.122
• Low-metallicity massive single stars with rotation. III. Source of ionization and C-IV emission in I Zw 18
• Mass Loss in 2D ZAMS Stellar Models
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• XTE J0111.2-7317 : a nebula-embedded X-ray binary in the SMC
• SN 2016iyc: A Type IIb supernova arising from a low-mass progenitor
• Discovery and origin of the radio emission from the multiple stellar system KQVel
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• Weak wind effects in CNO driven winds of hot first stars
• The Complex Upper HR Diagram
• The embedded clusters DBS 77, 78, 102, and 160-161 and their link with the interstellar medium
• Hot-star wind models with magnetically split line blanketing
• Looking for nebular He II emission south of the multiple-massive star system, HD 5980
• Diving into the magnetosphere of the Of?p star HD108
• Unveiling the evolutionary state of three B supergiant stars: PU Gem, $\epsilon$ CMa and $\eta$ CMa
• Eccentric grazing envelope evolution towards type IIb supernova progenitors
• Optically-thick Structure in Early B Type Supergiant Stellar Winds at Low Metallicities
• Evolution of Massive Stars along the Cosmic History
• Weighing stars from birth to death: mass determination methods across the HRD
• Local merger rates of double neutron stars
• A mixed helium-oxygen shell in some core-collapse supernova progenitors
• Are there magnetars in high-mass X-ray binaries?
• Stellar evolution, SN explosion, and nucleosynthesis
• X-Shooting ULLYSES: Massive stars at low metallicity. XIII. Putting the bi-stability jump to the test in the LMC
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• Characteristics and evolution of Be-type high mass X-ray binaries as potential Ultraluminous X-ray Sources
• An on-the-fly line-driven-wind iterative mass-loss estimator (LIME) for hot, massive stars of arbitrary chemical compositions
• Extremely iron-poor O-type stars in the Magellanic Bridge
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• Ultraviolet Spectropolarimetry with Polstar: Clumping and Mass-loss Rate Corrections
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material
• Untangling magnetic massive star properties with linear polarization variability and the Analytic Dynamical Magnetosphere model
• The evolution of planetary nebulae VI. On the chemical composition of the metal-poor PN G135.9+55.9
• Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
• Formation of millisecond pulsar-helium star binaries
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• Populations of ultraluminous X-ray sources in galaxies: origin and evolution
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• The rotational shear in pre-collapse cores of massive stars
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• Detection of extragalactic magnetic massive stars
• The colliding-wind binary HD 168112
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Investigation of [KSF2015] 1381-19L, a WC9-type star in the high extinction Galactic region
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• Probing Formation of Double Neutron Star Binaries around 1mHz with LISA
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• SN 2023ixf: interaction signatures in the spectrum at 445 days
• Population Synthesis of Gravitational Wave Sources
• Near-Eddington mass loss of hydrogen-rich Wolf-Rayet stars
• Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space
• Detection of a centrifugal magnetosphere in one of the most massive stars in the $\rho$ Oph star-forming cloud
• Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Origin of High Dark Remnant Fractions in Milky Way Globular Clusters: The Crucial Role of Initial Black Hole Retention
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• The wind properties of O-type stars at sub-SMC metallicity
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Mass fluxes for O-type supergiants with metallicity Z = Z_{\sun}/5
• New Insight into the FS CMa System MWC 645 from Near-Infrared and Optical Spectroscopy
• MOBSTER -- VII. Using light curves to infer magnetic and rotational properties of stars with centrifugal magnetospheres
• The X-ray binaries in M83: will any of them form gravitational wave sources for LIGO/VIRGO/KAGRA?
• $\delta$ Circini: A massive hierarchical triple system with an eclipsing binary
• The Predicted Properties of Helium-Enriched Globular Cluster Progenitors at High Redshift
• Spin-up and spin distribution of stellar black holes grown by gas accretion in proto-stellar clusters
• How many VHE gamma-ray binaries with young pulsars can be observed?
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
• Properties of dwarf stars in Cygnus OB2
• FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters
• WR 63: A multiple system (O+O)+WR ?
• The metallicity dependence of long-duration gamma-ray bursts
• The influence of rotation and metallicity on the explodability of massive stars
• Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter
• Sub-photospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves
• Transient star B/R ratio and star formation in $z\gtrsim 1$ lensed galaxies
• Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
• Power-law Emission-line Wings and Radiation-Driven Superwinds in Local Lyman Continuum Emitters
• First Stars. II. Evolution with mass loss
• Can circumstellar interaction explain the strange light curve features of Type Ib/c supernovae?
• Blue Loops, Cepheids, and Forays into Axions
• Investigation of the nature of the wind interaction in HD93205 based on multi-epoch X-ray observations
• A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow
• Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic technique
• Rare events of a peculiar thermonuclear supernova that precedes a core collapse supernova
• Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries
• Probing Thin Winds in Massive OB Stars of the SMC with JWST/NIRSPEC Br-alpha Spectroscopy
• Low-mass stellar and substellar candidate companions around massive stars in Sco OB1 and M17
• Observational Properties of $\beta$ Cephei Stars: 88 new samples discovered Based on TESS and Gaia Data
• Discovering Supernovae at Epoch of Reionization with Nancy Grace Roman Space Telescope
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Formation, diffusion and accreting pollution of DB white dwarfs
• Cyclic light variations and accretion disk evolution in the LMC eclipsing binary OGLE-LMC-DPV-062
• Dynamical double black holes and their host cluster properties
• Supernovae in colliding-wind binaries: observational signatures in the first year
• The Treasury of Extremely Metal-Poor O Stars
• Revisiting the Evolutionary Status of Massive Stars at the central parsec of the Milky Way
• 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
• SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
• HR-pyPopStar II: high spectral resolution evolutionary synthesis models low metallicity expansion and the properties of the stellar populations of dwarf galaxies
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• ALMA measurements of mass loss and wind clumping in the massive stars of the Arches cluster
• Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Massive star evolution revealed in the Mass-Luminosity plane
• Relative frequencies of core-collapse supernovae as a function of metallicity: observations vs theoretical predictions
• Self-lensing binaries as probes of Supernova physics
• Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes