Binary interaction dominates the evolution of massive stars

Abstract

The presence of a nearby companion alters the evolution of massive stars in binary systems, leading to phenomena such as stellar mergers, X-ray binaries and gamma-ray bursts. Unambiguous constraints on the fraction of massive stars affected by binary interaction were lacking. We simultaneously measured all relevant binary characteristics in a sample of Galactic massive O stars and quantified the frequency and nature of binary interactions. Over seventy per cent of all massive stars will exchange mass with a companion, leading to a binary merger in one third of the cases. These numbers greatly exceed previous estimates and imply that binary interaction dominates the evolution of massive stars, with implications for populations of massive stars and their supernovae.

9 page, 2 figures. This is the authors' version. Final version and supplementary materials available at http://www.sciencemag.org

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• Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system phi Persei
• Merging Black Holes in the Low-mass and High-mass Gaps from 2+2 Quadruple Systems
• Formation of Black Hole Low-Mass X-ray Binaries in Hierarchical Triple Systems
• Populations of stellar mass Black holes from binary systems
• MONOS: Multiplicity Of Northern O-type Spectroscopic systems. I. Project description and spectral classifications and visual multiplicity of previously known objects
• Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
• Hypervelocity runaways from the Large Magellanic Cloud
• Discovery of a magnetic field in the rapidly-rotating O-type secondary of the colliding-wind binary HD 47129 (Plaskett's star)
• Investigating the Binarity of S0-2: Implications for its Origins and Robustness as a Probe of the Laws of Gravity around a Supermassive Black Hole
• Luminous Red Novae: population models and future prospects
• The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems
• The binarity of Milky Way F,G,K stars as a function of effective temperature and metallicity
• Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
• Be discs in binary systems I. Coplanar orbits
• Fast radio bursts from activities of neutron stars newborn in BNS mergers: offset, birth rate and observational properties
• A VLT/FLAMES survey for massive binaries in Westerlund 1. IV. Wd1-5 - binary product and a pre-supernova companion for the magnetar CXOU J1647-45?
• Detecting Black Hole Binaries by Gaia
• Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution
• On the initial binary population for star cluster simulations
• Progenitors of Type IIb Supernovae: I. Evolutionary Pathways and Rates
• Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution
• Initial Mass Function Variations Cannot Explain the Ionizing Spectrum of Low Metallicity Starbursts
• The Habitable Exoplanet Observatory (HabEx) Mission Concept Study Interim Report
• The Tarantula Massive Binary Monitoring VI: Characterisation of hidden companions in 51 single-lined O-type binaries, a flat mass-ratio distribution, and black-hole binary candidates
• Supernova Remnants in the Local Group I: A model for the radio luminosity function and visibility times of supernova remnants
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
• 3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission
• Mapping Luminous Hot Stars in the Galaxy
• X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
• Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster
• The interaction of core-collapse supernova ejecta with a companion star
• Common-Envelope Episodes that lead to Double Neutron Star formation
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• An extremely energetic supernova from a very massive star in a dense medium
• On the kinematics of a runaway Be star population
• Exploring HeII$\lambda$1640 emission line properties at $z\sim 2-4$
• Stellar and nebular diagnostics in the UV for star-forming galaxies
• The Formation of Stellar Black Holes
• Black hole-neutron star mergers are unlikely multi-messenger sources
• Accreting black hole binaries in globular clusters
• The Close Binary Properties of Massive Stars in the Milky Way and Low-Metallicity Magellanic Clouds
• Discovery of tidally-perturbed pulsations in the eclipsing binary U Gru: a pioneering system for tidal asteroseismology
• Chirp Mass and Spin of Binary Black Holes from First Star Remnants
• Supernova 2010as: the Lowest-Velocity Member of a Family of Flat-Velocity Type IIb Supernovae
• The VLT-FLAMES Tarantula Survey XXVI: Properties of the O-dwarf population in 30 Doradus
• Binary Stars in the New Millennium
• Stripped-envelope supernova SN 2004dk is now interacting with hydrogen-rich circumstellar material
• Modelling Double Neutron Stars: Radio and Gravitational Waves
• Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type~II supernova progenitors
• The Nickel Mass Distribution of Stripped-Envelope Supernovae: Implications for Additional Power Sources
• The IACOB project. VII. The rotational properties of Galactic massive O-type stars revisited
• Hubble Tarantula Treasury Project. IV. The extinction law
• Investigating the diversity of supernovae type Iax: A MUSE and NOT spectroscopic study of their environments
• Complete ejection of OB stars from very young star clusters and the formation of multiple populations
• On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars
• Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• A solution to the proplyd lifetime problem
• Population synthesis of ultracompact X-ray binaries in the Galactic Bulge
• The progenitors of calcium-rich transients are not formed in situ
• Infrared identification of high-mass X-ray binaries discovered by INTEGRAL
• The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content
• An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS
• Gravitational Wave Astronomy With TianQin
• The supergiant B[e] star LHA 115-S 18 - binary and/or luminous blue variable?
• The Geometry and Dynamical Role of Stellar Wind Bubbles in Photoionised HII Regions
• The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A
• Double tidal disruptions in galactic nuclei
• State of the field: Binary black hole natal kicks and prospects for isolated field formation after GWTC-2
• Where are the double-degenerate progenitors of type Ia supernovae?
• Tomography of Massive Stars from Core Collapse to Supernova Shock Breakout
• The very young resolved stellar populations around stripped-envelope supernovae
• The young massive SMC cluster NGC 330 seen by MUSE II. Multiplicity properties of the massive-star population
• Resolved astrometric orbits of ten O-type binaries
• The Most Massive Heartbeat: An In-depth Analysis of ι Orionis
• Hoki: Making BPASS accessible through Python
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Circumstellar Interaction Powers the Light Curves of Luminous Rapidly Evolving Optical Transients
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• Angular momentum transport in massive stars and natal neutron star rotation rates
• Burst occurrence in young massive stellar objects
• Formation of wind-captured discs in Supergiant X-ray binaries : consequences for Vela X-1 and Cygnus X-1
• A new method for an objective, ${\chi }^2$-based spectroscopic analysis of early-type stars
• The IACOB project. VI. On the elusive detection of massive O-type stars close to the ZAMS
• Stellar Feedback and Resolved Stellar IFU Spectroscopy in the nearby Spiral Galaxy NGC 300
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• A nearby recent supernova that ejected the runaway star zeta Oph, the pulsar PSRB1706-16, and 60-Fe found on Earth
• Wolf-Rayet stars in the Small Magellanic Cloud as testbed for massive star evolution
• Highly Luminous Supernovae associated with Gamma-Ray Bursts I.: GRB 111209A/SN 2011kl in the Context of Stripped-Envelope and Superluminous Supernovae
• Evidence of magnetic field decay in massive main-sequence stars
• The closest black holes
• Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2 -- II. Resolved common proper motion pairs
• Electron Capture Supernovae From Close Binary Systems
• Population Synthesis of Black Hole Binaries with Normal-Star Companions: I. Detached Systems
• The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels
• Are Models for Core-Collapse Supernova Progenitors Consistent with the Properties of Supernova Remnants?
• Supernova Progenitors, Their Variability, and the Type IIP Supernova ASASSN-16fq in M66
• Wind-accreting Symbiotic X-ray Binaries
• Periodicity in Class II methanol masers in high mass star forming regions
• Resolving The Peak Of The Black Hole Mass Spectrum
• The early discovery of SN 2017ahn: signatures of persistent interaction in a fast declining Type II supernova
• Comprehensive study of ejecta-companion interaction for core-collapse supernovae in massive binaries
• On the accuracy of mass measurement for microlensing black holes as seen by Gaia and OGLE
• Are pulsars spun up or down by SASI spiral modes?
• Dynamics of jets during the Common Envelope phase
• Type Ia Supernova Sub-classes and Progenitor Origin
• In Search of the Thermal Eccentricity Distribution
• Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
• Discovery of $\beta$ Cep pulsations in the eclipsing binary V453 Cygni
• SPISEA: A Python-Based Simple Stellar Population Synthesis Code for Star Clusters
• Bow shock nebulae of hot massive stars in a magnetized medium
• The Origin of the Stellar Mass Distribution and Multiplicity
• Light Curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers
• The Origin of inequality: isolated formation of a 30+10Msun binary black-hole merger
• Velocity monitoring of gamma-Cas stars reveals their binarity status
• Rapidly evolving faint transients from stripped-envelope electron-capture supernovae
• The Tarantula Massive Binary Monitoring. IV. Double-lined photometric binaries
• The VLT-FLAMES Tarantula Survey. XXX. Red stragglers in the clusters Hodge 301 and SL 639
• Variability of Massive Stars with Known Spectral Types in the Small Magellanic Cloud Using 8 Years of OGLE-III Data
• Binary formation through gas-assisted capture and the implications for stellar, planetary and compact-object evolution
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• The spectroscopic Hertzsprung-Russell diagram of hot massive stars in the SMC
• The evolution of CNO elements in galaxies
• How much hydrogen is in Type Ib and IIb supernova progenitors?
• The Pre-Explosion Mass Distribution of Hydrogen-Poor Superluminous Supernova Progenitors and New Evidence for a Mass-Spin Correlation
• Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
• Dust in the wind: the role of recent mass loss in long gamma-ray bursts
• Kepler sheds new and unprecedented light on the variability of a blue supergiant: gravity waves in the O9.5Iab star HD 188209
• Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems
• Kepler's first view of O-star variability: K2 data of five O stars in Campaign 0 as a proof-of-concept for O-star asteroseismology
• Combined analysis of neutron star natal kicks using proper motions and parallax measurements for radio pulsars and Be X-ray binaries
• Evidence for quasi-chemically homogeneous evolution of massive stars up to solar metallicity
• Massive heartbeat stars from TESS. I. TESS sectors 1-16
• Runaway OB Stars in the Small Magellanic Cloud: Dynamical Versus Supernova Ejections
• Ultra Long Gamma-Ray Bursts from the collapse of Blue Super Giant stars: an end-to-end simulation
• The formation and coalescence sites of the first gravitational wave events
• Star cluster formation with stellar feedback and large-scale inflow
• Supernova axions convert to gamma-rays in magnetic fields of progenitor stars
• Massive Star Formation via the Collapse of Subvirial and Virialized Turbulent Massive Cores
• Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters
• Observational Inference on the Delay Time Distribution of Short Gamma-ray Bursts
• Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
• Discrepancies in the ages of young star clusters; evidence for mergers?
• Resolved Kinematics of Runaway and Field OB Stars in the Small Magellanic Cloud
• How fast do young star clusters expel their natal gas?: Estimating the upper limit of the gas expulsion time-scale
• On the origins of enigmatic stellar populations in Local Group galactic nuclei
• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
• Hypervelocity stars from young stellar clusters in the Galactic Centre
• The possible detection of a binary companion to a Type Ibn supernova progenitor
• The occurrence of nitrogen-enhanced metal-poor stars: implications for the initial mass function in the early Galactic halo
• Exploring the origin of magnetic fields in massive stars: II. New magnetic field measurements in cluster and field stars
• The Nearby Type Ibn Supernova 2015G: Signatures of Asymmetry and Progenitor Constraints
• STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
• Dynamics of binary black holes in low-mass young star clusters
• Detection of magnetic fields in both B-type components of the $\epsilon$ Lupi system: a new constraint on the origin of fossil fields?
• The Arches cluster revisited: I. Data presentation and stellar census
• Cas A and the Crab Were Not Stellar Binaries At Death
• Dark Passengers in Stellar Surveys
• Effective spin distribution of black hole mergers in triples
• The Initial Mass Function and the Surface Density Profile of NGC 6231
• All at once: transient pulsations, spin down and a glitch from the Pulsating Ultraluminous X-ray Source M82 X-2
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352
• Nucleosynthesis of binary-stripped stars
• Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations
• A Sample of OB Stars That Formed in the Field
• Prospects of Finding Detached Black Hole-Star Binaries with TESS
• Optical and IR observations of SN 2013L, a Type IIn Supernova surrounded by asymmetric CSM
• A transient radio source consistent with a merger-triggered core collapse supernova
• Radial abundance gradients in the outer Galactic disk as traced by main-sequence OB stars
• Double neutron star mergers from hierarchical triple-star systems
• The population of white dwarf-main sequence binaries in the SDSS DR 12
• The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population
• When H II Regions are Complicated: Considering Perturbations from Winds, Radiation Pressure, and Other Effects
• Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia
• The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase
• The observed vs total population of ULXs
• Gaia pulsars and where to find them
• Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
• Multiplicity of Galactic Luminous Blue Variable stars
• Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
• Resolving the kinematics of the disks around Galactic B[e] supergiants
• Dynamical evolution of Population III stellar systems and the resulting binary statistics
• Impact of binary interactions on the diffuse supernova neutrino background
• A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• The multiplicity fraction in 202 open clusters from Gaia
• The Red Supergiant Content of M31 and M33
• Isolated massive stars in the Galactic center: The dynamic contribution from the Arches and Quintuplet star clusters
• A dearth of short-period massive binaries in the young massive star forming region M17: Evidence for a large orbital separation at birth?
• Revisiting the Impact of Dust Production from Carbon-Rich Wolf-Rayet Binaries
• It's written in the massive stars: The role of stellar physics in the formation of black holes
• A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. I. The northern WC sequence
• Nebular emission from young stellar populations including binary stars
• A 1.05 $M_{\odot }$ Companion to PSR J2222-0137: The Coolest Known White Dwarf?
• Catching a star before explosion: the luminous blue variable progenitor of SN 2015bh
• Galactic runaway O and Be stars found using Gaia DR3
• Population Synthesis of Galactic Be-star Binaries with A Helium-star Companion
• Seven years of coordinated Chandra-NuSTAR observations of SN2014C unfold the extreme mass-loss history of its stellar progenitor
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• Binary Properties from Cepheid Radial Velocities (CRaV)
• White dwarf masses in cataclysmic variables
• Comparison of the optical light curves of hydrogen-rich and hydrogen-poor type II supernovae
• Black hole spins in coalescing binary black holes
• Population synthesis of accreting white dwarfs: II. X-ray and UV emission
• The Formation of Very Massive Stars
• The delayed time distribution of massive double compact star mergers
• Confusing binaries: the role of stellar binaries in biasing disk properties in the Galactic Center
• The IRX-$\beta$ relation of high-redshift galaxies
• Nearby supernova host galaxies from the CALIFA Survey: II. SN environmental metallicity
• The mass of the very massive binary WR21a
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• Multiple Star Systems in the Orion Nebula
• GW150914-like Black Holes as Galactic High-Energy Sources
• Constraints on single-degenerate Chandrasekhar mass progenitors of Type Iax supernovae
• An updated stellar census of the Quintuplet cluster
• The CubeSpec space mission. I. Asteroseismology of massive stars from time series optical spectroscopy: science requirements and target list prioritisation
• Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants
• Supernovae in the Central Parsec: A Mechanism for Producing Spatially Anisotropic Hypervelocity Stars
• Numerical experiments to help understand cause and effect in massive star evolution
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Binarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC
• A Rare Encounter with Very Massive Stars in NGC 3125-A1
• The Outcome of Supernovae in Massive Binaries; Removed Mass, and its Separation Dependence
• High-mass pulsators in eclipsing binaries observed using TESS
• The nature of the bright ULX X-2 in NGC3921: a Chandra position and HST candidate counterpart
• Aluminium-26 from massive binary stars I: non-rotating models
• On the rates of type Ia supernovae originating from white dwarf collisions in quadruple star systems
• Comparing Compact Object Distributions from Mass- and Presupernova Core Structure-based Prescriptions
• A synthetic model of the gravitational wave background from evolving binary compact objects
• Stripped-envelope core-collapse supernova ${}^{56}$Ni masses: Persistently larger values than supernovae type II
• A magnetic massive star has experienced a stellar merger
• Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae
• A sequence of Type Ib, IIb, II-L, and II-P supernovae from binary-star progenitors of varying initial separation
• Non-interacting black hole binaries with Gaia and LAMOST
• Do the majority of stars form as gravitationally unbound?
• Implementing Primordial Binaries in Simulations of Star Cluster Formation with a Hybrid MHD and Direct N-Body Method
• On the stability and collisions in triple stellar systems
• Magnetic fields driven by tidal mixing in radiative stars
• 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
• The binarity of Galactic dwarf stars along with effective temperature and metallicity
• Progenitor Mass Distribution of Core-Collapse Supernova Remnants in Our Galaxy and Magellanic Clouds based on Elemental Abundances
• High-resolution spectroscopy of SN 2017hcc and its blueshifted line profiles from post-shock dust formation
• Detecting Accelerating Eccentric Binaries in the LISA Band
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• Binary mass ratios: system mass not primary mass
• X-ray Emission from Eta Carinae near Periastron in 2009 I: A Two State Solution
• Massive stars in the hinterland of the young cluster, Westerlund 2
• A New Class of Nascent Eclipsing Binaries with Extreme Mass Ratios
• Evolution of massive stellar triples and implications for compact object binary formation
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• Mass discrepancy analysis for a select sample of Type II-Plateau supernovae
• Nonconservative Mass Transfer in Massive Binaries and the Formation of Wolf-Rayet+O Binaries
• Reddening, Distance, and Stellar Content of the Young Open Cluster Westerlund 2
• Slow ionized wind and rotating disklike system associated with the high-mass young stellar object G345.4938+01.4677
• Explaining the differences in massive star models from various simulations
• Stars and gas in the most metal-poor galaxies I: COS and MUSE observations of SBS 0335-052E
• On the formation and evolution of the first Be star in a black hole binary MWC 656
• Constraining the Overcontact Phase in Massive Binary Evolution I. Mixing in V382 Cyg, VFTS 352, and OGLE SMC-SC10 108086
• Stellar Binaries That Survive Supernovae
• Observational Properties of Type Ib/c Supernova Progenitors in Binary Systems
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• The cosmic carbon footprint of massive stars stripped in binary systems
• A close encounter of the massive kind
• Spectroscopic characterization of the known O-star population in Cygnus OB2. Evidence of multiple star-forming bursts
• Binary evolution, gravitational-wave mergers and explosive transients in multiple-populations gas-enriched globular-clusters
• An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion
• Star formation history of the solar neighbourhood as told by Gaia
• SN2012ab: A Peculiar Type IIn Supernova with Aspherical Circumstellar Material
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• A beta Cephei pulsator and a changing orbital inclination in the high-mass eclipsing binary system VV Orionis
• Constraints on the Binary Companion to the SN Ic 1994I Progenitor
• Interferometric detections of sdO companions orbiting three classical Be stars
• Forming Pop III binaries in self-gravitating disks: how to keep the orbital angular momentum
• The Betelgeuse Project: Constraints from Rotation
• Return of the TEDI: revisiting the Triple Evolution Dynamical Instability channel in triple stars
• Unlocking Galactic Wolf-Rayet stars with $\text{Gaia}$ DR2 II: Cluster and Association membership
• The multiplicity of massive stars: a 2016 view
• HR 6819 is a binary system with no black hole -- revisiting the source with infrared interferometry and optical integral field spectroscopy
• The Keplerian three-body encounter I. Insights on the origin of the S-stars and the G-objects in the Galactic center
• The diversity of supernovae and impostors shortly after explosion
• The Shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system
• Early-type Eclipsing Binaries with Intermediate Orbital Periods
• Blue supergiants as descendants of magnetic main sequence stars
• The isolation of Luminous Blue Variables: On subdividing the sample
• Modelling Type Ic Supernovae with TARDIS: Hidden Helium in SN1994I?
• Dynamics of a Massive Binary at Birth
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• The VLT-FLAMES Tarantula Survey: XXXI. Radial velocities and multiplicity constraints of red supergiant stars in 30 Doradus
• A pilot survey of the binarity of Massive Young Stellar Objects with $K$ band adaptive optics
• Is Betelgeuse the Outcome of a Past Merger?
• Progenitor Mass Distribution for Core-Collapse Supernova Remnants in M31 and M33
• Massive pre-main sequence stars in M17
• Low-metallicity massive single stars with rotation. II. Predicting spectra and spectral classes of chemically-homogeneously evolving stars
• First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics
• An Observationally-Derived Kick Distribution for Neutron Stars in Binary Systems
• An Optical and Infrared Photometric Study of the Young Open Cluster IC 1805 in the Giant H II Region W4
• Stars stripped in binaries -- the living gravitational wave sources
• A relation between the radial velocity dispersion of young clusters and their age: Evidence for hardening as the formation scenario of massive close binaries
• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
• Binary companions of nearby supernova remnants found with Gaia
• An investigation into the fraction of particle accelerators among colliding-wind binaries. Towards an extension of the catalogue
• Two spotted and magnetic early B-type stars in the young open cluster NGC2264 discovered by MOST and ESPaDOnS
• The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A
• No surviving stellar companion for Cassiopeia A
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• The Red Supergiant Binary Fraction as a Function of Metallicity in M31 and M33
• Black hole - black hole total merger mass and the origin of LIGO/Virgo sources
• Circumstellar discs in Galactic centre clusters: Disc-bearing B-type stars in the Quintuplet and Arches clusters
• A partially stripped massive star in a Be binary at low metallicity: A missing link towards Be X-ray binaries and double neutron star mergers
• Massive binary star mergers in galactic nuclei: implications for blue stragglers, binary S-stars and gravitational waves
• HV2112, a Thorne-Zytkow Object or a Super Asymptotic Giant Branch Star
• Collapsar Black Holes are Likely Born Slowly Spinning
• Dispersion and Rotation Measures from the Ejecta of Compact Binary Mergers: Clue to the Progenitors of Fast Radio Bursts
• Black Hole/Pulsar Binaries in the Galaxy
• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
• Binary Red Supergiants II: Discovering and Characterizing B-type Companions
• The Impact of Feedback in Massive Star Formation. II. Lower Star Formation Efficiency at Lower Metallicity
• Calibration of neutron star natal kick velocities to isolated pulsar observations
• The impact of primordial binary on the dynamical evolution of intermediate massive star clusters
• Massive binary black holes from Population II and III stars
• Progenitors of Type IIb Supernovae: II. Observable Properties
• Formation Timescales for High-Mass X-ray Binaries in M33
• Very massive stars in not so massive clusters
• Recent Star Formation in the Leading Arm of the Magellanic Stream
• The first gravitational-wave burst GW150914, as predicted by the scenario machine
• Modelling nova populations in galaxies
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Low-mass X-ray binaries from black-hole retaining globular clusters
• Modeling X-ray binary evolution in normal galaxies: Insights from SINGS
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
• An ALMA 3mm continuum census of Westerlund 1
• The occurrence of classical Cepheids in binary systems
• A systematic reclassification of type IIn supernovae
• The impact of realistic red supergiant mass-loss on stellar evolution
• Neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy superluminous supernovae and Thorne-Żytkow objects
• AGB winds in interacting binary stars
• Wide binary companions to massive stars and their use in constraining natal kicks
• The multiplicity of massive stars in the Orion Nebula cluster as seen with long-baseline interferometry
• Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Numerically Modeling the First Peak of the Type IIb SN 2016gkg
• Core-collapse supernova progenitor constraints using the spatial distributions of massive stars in local galaxies
• Planet Hunters X: Searching for Nearby Neighbors of 75 Planet and Eclipsing Binary Candidates from the K2 Kepler Extended Mission
• A high mass progenitor for the Type Ic Supernova 2007gr inferred from its environment
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Testing the fossil field hypothesis: could strongly magnetised OB stars produce all known magnetars?
• Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants
• Data-driven spectroscopic estimates of absolute magnitude, distance and binarity -- method and catalog of 16,002 O- and B-type stars from LAMOST
• A solar-type star polluted by calcium-rich supernova ejecta inside the supernova remnant RCW 86
• Binary Red Supergiants: A New Method for Detecting B-type Companions
• Case A and B evolution towards electron capture supernova
• Nothing to see here: Failed supernovae are faint or rare
• Multiplicity of the red supergiant population in the young massive cluster NGC 330
• ZFIRE: Using H$\alpha$ equivalent widths to investigate the in situ initial mass function at z~2
• 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
• X-ray properties of early-type stars in the Tarantula Nebula from T-ReX
• Cepheids with giant companions. I. Revealing a numerous population of double-lined binary Cepheids
• A High-Resolution Multiband Survey of Westerlund 2 With the Hubble Space Telescope. III. The present-day stellar mass function
• Properties of six short-period massive binaries: a study of the effects of binarity on surface chemical abundances
• Extreme mass-ratio gravitational-wave sources: Mass segregation and post binary tidal-disruption captures
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars: II. The northern WNE sequence
• The gravitational-wave signal generated by a galactic population of double neutron-star binaries
• Observational signatures of past mass-exchange episodes in massive binaries: The case of HD 149 404
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution -- Insights from the IRAM NOEMA large program CORE
• The Value-Added Catalog of ASAS-SN Eclipsing Binaries: Parameters of Thirty Thousand Detached Systems
• The B-type Binaries Characterisation Programme II. VFTS 291: A stripped star from a recent mass transfer phase
• Evaluating the impact of binary parameter uncertainty on stellar population properties
• Apsidal motion in the massive binary HD152218
• Search Instructions for Globular Clusters in Formation at High Redshifts
• Close Encounters of Wide Binaries Induced by the Galactic Tide: Implications for Stellar Mergers and Gravitational-Wave Sources
• The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?
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• The First Metallicity Study of M83 using the integrated UV light of Star Clusters
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• Carbon Abundances in Starburst Galaxies of the Local Universe
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• Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen: Image of the close companion in front of the primary
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• A census of OBe stars in nearby metal-poor dwarf galaxies reveals a high fraction of extreme rotators
• The role of stellar expansion on the formation of gravitational wave sources
• The Carnegie Supernova Project II. Observations of the intermediate luminosity red transient SNhunt120
• The First Dynamical Mass Determination of a Nitrogen-rich Wolf-Rayet Star using a Combined Visual and Spectroscopic Orbit
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• The variability of the BRITE-est Wolf-Rayet binary, ${\gamma }^2$ Velorum I. Photometric and spectroscopic evidence for colliding winds
• Spectroscopic patch model for massive stars using PHOEBE II and FASTWIND
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• Confirming NGC 6231 as the parent cluster of the runaway high-mass X-ray binary HD 153919/4U 1700-37 with Gaia DR2
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• Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022
• CPD-64 2731: a massive spun-up and rejuvenated high-velocity runaway star
• Inferring the progenitor mass-kinetic energy relation of stripped-envelope core-collapse supernovae from nebular spectroscopy
• The Extremely Metal-Poor SN 2023ufx: A Local Analog to High-Redshift Type II Supernovae
• The Betelgeuse Project III: Merger Characteristics
• Modeling the Optical to Ultraviolet Polarimetric Variability from Thomson Scattering in Colliding Wind Binaries
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• Numerical Modelling of Tertiary Tides
• Electromagnetic transients and gravitational waves from white dwarf disruptions by stellar black holes in triple systems
• A probable pre-main sequence chemically peculiar star in the open cluster Stock 16
• R144 : a very massive binary likely ejected from R136 through a binary-binary encounter
• High-spatial-resolution simulations of Be star disks in binary systems: I. Structure and kinematics of coplanar disks
• Primordial mass segregation of star clusters with primordial binaries
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• Galactic population of black holes in detached binaries with low-mass stripped helium stars: the case of LB-1 (LS~V+22~25)
• Eclipsing high-mass binaries I. Light curves and system parameters for CPD-518946, PISMIS24-1 and HD319702
• GABE: Galaxy Assembly with Binary Evolution
• Luminous Blue Variables
• Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud
• Neutron stars in accreting systems -- signatures of the QCD phase transition
• Monte Carlo simulations of multiple populations in globular clusters: constraints on the initial size of the second generation from binary stars
• Scalable stellar evolution forecasting: Deep learning emulation vs. hierarchical nearest neighbor interpolation
• A study of the F-giant star $\theta$ Scorpii A: a post-merger rapid rotator?
• The long-period massive binary HD~54662 revisited
• WR + O binaries as probes of the first phase of mass transfer
• The winking eye of a very massive star: WR 21a revealed as an eclipsing binary by TESS
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• An interferometric study of B star multiplicity
• Discovery of Magnetospheric Interactions in the Doubly-Magnetic Hot Binary $\epsilon$ Lupi
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• Wind Collision and Accretion Simulations of the Massive Binary System HD 166734
• The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
• Investigating the Circumstellar Disk of the Be Shell Star 48 Librae
• Analytic approximations for massive close post-mass transfer binary systems
• UVIT Study of the MAgellanic Clouds (U-SMAC) II. A Far-UV catalog of the Small Magellanic Cloud: Morphology and Kinematics of young stellar population
• Fast radio bursts at the dawn of the 2020s
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
• BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
• To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars
• Ionizing stellar population in the disc of NGC 3310 - II. The Wolf-Rayet population
• Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
• Massive young stellar objects in the Local Group spiral galaxy M33 identified using machine learning
• A Search for Unbound Stellar Companions to Pulsar J1124-5916
• Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
• The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems
• The IACOB project XIV. New clues on the location of the TAMS in the massive star domain
• X-Shooting ULLYSES: Massive Stars at Low Metallicity: XI. Pipeline-determined Physical Properties of Magellanic Cloud OB Stars
• The spectroscopic binary fraction of the young stellar cluster M17
• Investigating the observational properties of Type Ib supernova SN 2017iro
• Kinematics of Luminous Blue Variables in the Large Magellanic Cloud
• L-GALAXIES 2020: The formation and chemical evolution of stellar haloes in Milky Way Analogues and galaxy clusters
• Ultraviolet Spectropolarimetry:Conservative and Nonconservative Mass Transfer in OB Interacting Binaries
• Black holes at cosmic dawn in the redshifted 21cm signal of HI
• Accretion induced black hole spin up revised by numerical GR MHD simulations
• Wide binary pulsars from electron-capture supernovae
• Progenitors of Long-Duration Gamma-ray Bursts
• 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
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• Long gamma ray burst rate in the binary merger progenitor model
• Do individual Spitzer young stellar object candidates enclose multiple UKIDSS sources?
• Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
• Near-infrared spectroscopy of 20 new Chandra sources in the Norma Arm
• An Argument for Weakly-Magnetized, Slowly-Rotating Progenitors of Long Gamma-Ray Bursts
• Numerical Tests of Rotational Mixing in Massive Stars with the new Population Synthesis Code BONNFIRES
• Autonomous Disentangling for Spectroscopic Surveys
• The onset of stellar multiplicity in massive star formation: A search for low-mass companions of massive young stellar objects with $L^{\prime }$-band adaptive optics imaging
• The spatial distributions of blue main-sequence stars in Magellanic Cloud star clusters
• Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
• Binary imposters: Mergers in massive hierarchical triple stars
• A binary origin for the first isolated stellar-mass black hole detected with astrometric microlensing
• A Be Star + He Star Binary as an Indicator of a Binary Mass Transfer Phase
• The First Candidate Colliding-Wind Binary in M33
• Tying the geometrical traits of massive young stellar objects and their discs to a potential evolutionary sequence using infrared observations
• The mass distribution of stellar mergers: A new scenario for several FS CMa stars
• Gravitational Wave Sources from Pop III Stars are Preferentially Located within the Cores of their Host Galaxies
• Formation rate of LB-1-like systems through dynamical interactions
• Statistics of Magrathea exoplanets beyond the Main Sequence. Simulating the long-term evolution of circumbinary giant planets with TRES
• Accurate fundamental parameters and distance to a massive early-type eclipsing binary in the Danks 2 cluster
• Five years of BRITE-Constellation photometry of the luminous blue variable P Cygni: properties of the stochastic low-frequency variability
• UV Spectropolarimetry with Polstar: Massive Star Binary Colliding Winds
• On the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth
• Rethinking mass transfer: a unified semi-analytical framework for circular and eccentric binaries. I. Orbital evolution due to conservative mass transfer
• The mass distribution of the first stars can be determined via the 21-cm signal
• Thermal generation of the magnetic field in the surface layers of massive stars
• The Formation of Electron-capture Supernovae: A Review
• Unveiling the architecture of a pulsar - binary black-hole triple system with pulsar arrival time analysis
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Astrometric mass measurement of compact companions in binary systems with Gaia
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• The fate of rotating massive stars across cosmic times
• VFTS 243 as predicted by the BPASS fiducial models
• Discovery and Characterization of a Rare Magnetic Hybrid $\beta$ Cephei Slowly Pulsating B-type Star in an Eclipsing Binary in the Young Open Cluster NGC 6193
• Gravitational Waves from Mirror World
• Magnetic Webs in Stellar Radiative Zones
• On the star formation efficiencies and evolution of multiple stellar generations in Globular Clusters
• The ionizing sources of luminous compact HII regions in the RCW106 and RCW122 clouds
• LAMOST J040643.69+542347.8: the fastest Rotator in the Galaxy
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Natal kicks of compact objects
• Massive stars, successes and challenges
• Ellipsars: Ring-like explosions from flattened stars
• X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
• HIP 15429: A newborn Be star on an eccentric binary orbit
• Formation of the First Two Black Hole-Neutron Star Mergers (GW200115 and GW200105) from Isolated Binary Evolution
• Population and spectral synthesis: it doesn't work without binaries
• Effects of binary stellar populations on direct collapse black hole formation
• Effects of physical conditions on the stellar initial mass function: The low-metallicity star-forming region Sh 2-209
• The origins of low-luminosity supernovae: the case of SN 2016bkv
• Candidate Young Stellar Objects in the S-cluster: The Kinematic Analysis of a Sub-population of the Low-mass G-objects close to Sgr A*
• Investigating the UV-excess in star clusters with $N$-body simulations: predictions for future CSST observations
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system $\epsilon$ Lupi
• Radio stars of the SKA
• On the mass-function of GWTC-2 binary black hole systems and their progenitors
• Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve
• An upper limit on the frequency of short-period black hole companions to Sun-like stars
• LIFELINE: The program for the simulation of the X-ray line profiles in massive colliding wind binaries
• Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole
• VLT/MUSE and ATCA observations of the host galaxy of the short GRB 080905A at z=0.122
• Infrared Observations of the Quintuplet Proper Members using SOFIA/FORCAST and Gemini/TReCS
• Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes
• Progenitor constraints for core-collapse supernovae from Chandra X-ray observations
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum
• Low-metallicity massive single stars with rotation. III. Source of ionization and C-IV emission in I Zw 18
• Weighing stars from birth to death: mass determination methods across the HRD
• Dust around massive stars is agnostic to galactic environment: New insights from PHAT/BEAST
• Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. III. Evolution
• Exploring GRBs and supernovae connection: does a superluminous hypernova population exist?
• The Location of Young Pulsar PSR J0837$-$2454: Galactic Halo or Local Supernova Remnant?
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor
• The binary fraction of Blue Horizontal-Branch (BHB) Stars
• Evidence for the Keplerian orbit of a close companion around a giant star
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• The non-thermal emission from the colliding-wind binary Apep
• Digging into the Interior of Hot Cores with ALMA (DIHCA). VII. Disk candidates around high-mass stars and evidence of anisotropic infall
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• An observational study of rotation and binarity of Galactic O-type runaway stars
• Multiple variability time-scales of the early nitrogen-rich Wolf-Rayet star WR7
• New Massive Contact Twin Binary in a Radio-quiet HII Region Associated with the M17 Complex
• Searching for compact objects in the single-lined spectroscopic binaries of the young Galactic cluster NGC 6231
• The Small Separation A-Star Companion Population: First Results with CHARA/MIRC-X
• Merger Conditions of Population III Protostar Binaries
• The long-term evolution of main-sequence binaries in DRAGON simulations
• Massive stellar triples on the edge: A numerical study of the evolution and final outcomes of destabilized massive triples
• X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
• New insight into the massive eccentric binary HD 165052: self-consistent orbital solution, apsidal motion, and fundamental parameters
• Gaia-ESO Survey: massive stars in the Carina Nebula. II. The spectroscopic analysis of the O-star population
• Spindown of massive main sequence stars in the Milky Way
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
• Period change of massive binaries from combined photometric and spectroscopic data in Cygnus OB2
• Rotational synchronisation of B-type binaries in 30 Doradus
• LBV phenomenon and binarity: The environment of HR Car
• A recent history of science cases for interferometry
• Betelgeuse, the Prototypical Red Supergiant
• Betelgeuse's Buddy: X-Ray Constraints on the Nature of $\alpha$ Ori B
• Binary stellar evolution yields in galactic chemical evolution calculations
• Binarity at LOw Metallicity (BLOeM): Bayesian inference of natal kicks from inert black hole binaries
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• Power density spectra morphologies of seismically unresolved red-giant asteroseismic binaries
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• The evolutionary and asteroseismic imprints of mass accretion. The 10 M${}_{\odot }$ $\beta$ Cep case study
• Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
• The Complex Circumstellar and Circumbinary Environment of V356 Sgr
• Probing Massive Stars Around Gamma-Ray Burst Progenitors
• Observation of double star by long-baseline interferometry
• How Rotation Affects Masses and Ages of Classical Cepheids
• Two New Rapidly-Rotating ON Stars Found With LAMOST
• Study of the Galactic radio sources in the SCORPIO survey resolved by ATCA at 2.1 GHz
• Revealing Double White Dwarf Mergers with Multi-messenger Signals
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• A Global Census of Metals in the Universe
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• A High Angular Resolution Survey of Massive Stars in Cygnus OB2: $JHK$ Adaptive Optics Results from the Gemini Near-InfraRed Imager
• Neutron star binaries produced by binary-driven hypernovae, their mergers, and the link between long and short GRBs
• The nature of the Cygnus extreme B-supergiant 2MASS J20395358+4222505
• Local merger rates of double neutron stars
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• On the relationship between metallicity distributions of globular clusters and of circumgalactic gas
• Stellar evolution, SN explosion, and nucleosynthesis
• LAMOST medium-resolution spectroscopic survey of binarity and exotic star (LAMOST-MRS-B): Observation strategy and target selection
• Two circumstellar nebulae discovered with the Wide-field Infrared Survey Explorer and their massive central stars
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• Probing the detectability of electromagnetic signatures from Galactic isolated black holes
• Constraints on Explosion Timescale of Core-Collapse Supernovae Based on Systematic Analysis of Light Curves
• Binarity of the LBV HR Car
• Ultraluminous X-ray sources in Globular Clusters
• Mass loading of outflows from evolving Young Massive Clusters
• Coaxing the Eclipsing Binary V367 Cygni Out of Its Shell
• The Dynamical Evolution of Multiple Systems of Trapezium Type
• The bright long-lived Type II SN 2021irp powered by aspherical circumstellar material interaction (II): Estimating the CSM mass and geometry with polarimetry and light curve modeling
• Numerical simulations of wind-equatorial gas interaction in eta Carinae
• Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-7219
• Gravitational wave backgrounds from coalescing black hole binaries at cosmic dawn: an upper bound
• Surprises from the spins: astrophysics and relativity with detections of spinning black-hole mergers
• Short and long term evolution of a stellar disk around a massive black hole: The role of binaries, the cusp and stellar evolution
• Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• Quantitative spectroscopy of multiple OB stars: I. The quadruple system HD 37061 at the centre of Messier 43
• The near-infrared companion to HD94660 (=KQ Vel)
• Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
• Hot Stars in the GALEX Ultraviolet Sky Surveys (GUVcat_AISxSDSS_HS) and the Binary Fraction of Hot Evolved Stars
• The potential of space observations for pulsating pre-main sequence stars
• Fundamental parameters of the massive eclipsing binary HM1 8
• Global Stellar Budget for LIGO Black Holes
• CHARA/MIRC-X -- a high-sensitive six telescope interferometric imager concept, commissioning, and early science
• Impact of Population III stars on the astrophysical gravitational-wave background
• The rotational shear in pre-collapse cores of massive stars
• The Signature of a Windy Radio Supernova Progenitor in a Binary System
• Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
• Reconstructing EUV spectrum of star forming regions from millimeter recombination lines of HI, HeI, and HeII
• An optimal envelope ejection efficiency for merging neutron stars
• Two twin binaries with nearly identical components: KIC 4826439 and KIC 6045264
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Thorne-Żytkow Objects
• Magnetic Fields in Stars: Origin and Impact
• Probing the models: Abundances for high-mass stars in binaries
• Painting a Family Portrait of the Yellow Super- and Hypergiants in the Milky Way I. Constraining the Distances and Luminosities
• The bound origin of low-mass stellar binaries
• The Binary Fraction of B-type Runaway Stars from LAMOST DR8
• Supernovae in massive binaries and compact object mergers near supermassive black holes
• Wray 15-906: a candidate luminous blue variable discovered with WISE, Herschel and SALT
• TYCHO -- Realistically Simulating Exoplanets within Stellar Clusters I: Improving the Monte Carlo Approach
• Spectropolarimetry of stars across the H-R diagram
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• A stringent upper limit on Be star fractions produced by binary interaction
• The observed multiplicity properties of B-type stars in the Galactic young open cluster NGC 6231
• The Relative Calibration of Radial Velocity for LAMOST Medium Resolution Stellar Spectra
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• The Red Supergiant Content of the Local Group
• MoBiDICT: new 3D static models of close, synchronized binaries in hydrostatic equilibrium
• Monitoring the X-ray Variability of Bright X-ray Sources in M33
• Explanations for the two-component spectral energy distributions of gravitationally lensed stars at high redshifts
• Type Ia Supernovae from First-generation Stars
• Chemical enrichment by collapsars as the origin of the unusually high [Ba/Fe] in a massive star cluster of the dwarf galaxy NGC 1569
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Red supergiant stars in binary systems II. Confirmation of B-type companions of red supergiants in the Small Magellanic Cloud using Hubble ultra-violet spectroscopy
• Population Synthesis of Gravitational Wave Sources
• The nature of the X-ray pulsar in M31: an intermediate mass X-ray binary?
• Supernova explosions of runaway stars and young neutron stars above the Galactic plane
• Red Supergiants -- The Other Side of the H-R Diagram
• Red Supergiants in the Milky Way and Nearby Galaxies
• Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star Zeta Oph from high-cadence ESPRESSO spectroscopy and TESS photometry
• SXP7.92: A Recently Rediscovered Be/X-ray Binary in the Small Magellanic Cloud, Viewed Edge On
• SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction
• Observed Consequences of Presupernova Instability in Very Massive Stars
• The VLT-Flames Tarantula Survey: an overview of the VFTS results so far
• Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
• The wind properties of O-type stars at sub-SMC metallicity
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• The YMDB catalog: Young massive detached binaries for the determination of high-precision absolute stellar parameters
• WR 63: A multiple system (O+O)+WR ?
• Cosmic Radioactivity and Galactic Chemical Evolution
• $\delta$ Circini: A massive hierarchical triple system with an eclipsing binary
• High-mass stars in Milky Way clusters
• Double white dwarf binary population in MOCCA star clusters -- Comparisons with observations of close and wide binaries
• Revisiting the orbital motion of WR 138
• Fading Echoes of Interaction: Probing Centuries of Preexplosion Mass-Loss in Four Type IIn Supernovae
• MONOS: Multiplicity Of Northern O-type Spectroscopic systems. III. New orbits and Gaia TESS analysis for 10 SB2E systems
• Discovery of a 310-day Period from the Enshrouded Massive System NaSt1 (WR 122)
• Interaction of a high-mass X-ray binary with the interstellar medium through stellar wind. The case of GX 301-2
• Supernova interaction with dense mass loss
• The explosive life of massive binaries
• Modeling the circumstellar interaction around SN 2004gq
• Can circumstellar interaction explain the strange light curve features of Type Ib/c supernovae?
• Primordial mass segregation of star clusters: The role of binary stars
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• The X-ray binaries in M83: will any of them form gravitational wave sources for LIGO/VIRGO/KAGRA?
• Red Variable Stars in Three M81 Group Dwarf Galaxies
• Nuclear astrophysics
• Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
• A Fundamental Plane in X-ray Binary Activity of External Galaxies
• Synchrotron Radio Emission as a Proxy to Identify Long Period Massive Binaries
• Neutrinos from Diffuse Supernova Background
• The influence of rotation and metallicity on the explodability of massive stars
• Constraining the quantum gravity polymer scale using LIGO data
• 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
• Low-mass stellar and substellar candidate companions around massive stars in Sco OB1 and M17
• Mergers of binary neutron star systems: a multi-messenger revolution
• Massive stars in the Tarantula Nebula: A Rosetta Stone for Extragalactic Supergiant HII Regions
• Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
• Interpreting Galaxy Properties with Improved Modelling
• How many VHE gamma-ray binaries with young pulsars can be observed?
• Spatially resolved centrifugal magnetosphere caught in motion around the secondary component of $\rho$ Oph A
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars
• A low mass, binary-stripped envelope for the Type IIb SN 2024abfo
• Fundamental parameters of the eclipsing binary DD CMa and evidence for mass exchange
• Radiation-Driven Warping of Circumbinary Disks Around Eccentric Young Star Binaries
• Detection and characterisation of two VLM binaries: LP 1033-31 and LP 877-72
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• The Age of the R127 & R128 Clusters: Implications for the LBV
• Evolving Low- and Intermediate-Mass Binaries: Departures from Classical Theory
• Viscous and centrifugal instabilities of massive stars
• Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness
• Advanced Astroinformatics for Variable Star Classification
• Zeta-Payne: a fully automated spectrum analysis algorithm for the Milky Way Mapper program of the SDSS-V survey
• Low-frequency spectra of neutron star + OB supergiant binaries: Does wind density drive persistent and flaring modes of accretion?
• The Formation of Globular Clusters as a Case of Overcooling
• Constraining Black Hole Natal Kicks with Astrometric Microlensing
• A solution to the paradox of youth in the Galactic centre
• The Sejong Open Cluster Survey (SOS). VII. A Photometric Study of the Young Open Cluster IC 1590
• Hubble Space Telescope Snapshot Survey for Resolved Companions of Galactic Cepheids: Final Results
• The interaction of core-collapse supernova ejecta with a stellar companion
• Non-parametric identification of single-lined binary candidates in young clusters using single-epoch spectroscopy
• Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST
• Merging massive black holes: the right place and the right time
• Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey
• Massive Star Formation in the Ultraviolet Observed with the Hubble Space Telescope
• New Blue and Red Variable Stars in NGC 247
• Massive stars evolution: feedbacks in low-Z environment
• Accretion in massive colliding wind binaries and the effect of wind momentum ratio
• The impact of ultraviolet suppression on the rates and properties of strongly lensed Type IIn supernovae detected by LSST
• A method for statistical research on binary stars using radial velocities
• The Carina High-Contrast Imaging Project for massive Stars (CHIPS) I. Methodology and proof of concept on QZ Car ($\equiv$ HD93206)
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• SN 2024hpj: A perspective on SN 2009ip-like events
• Astrophotometric search for massive stars in the Milky way. Confronting Random Forest predictions with available spectroscopy
• The Role of High-mass Stellar Binaries in the Formation of High-mass Black Holes in Dense Star Clusters
• Constraining the Variability and Binary Fraction of Galactic Center Young Stars
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Self-lensing binaries as probes of Supernova physics
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• The Progenitor of the S147 Supernova Remnant
• The Fast Radio Burst-emitting magnetar SGR 1935+2154 -- proper motion and variability from long-term Hubble Space Telescope monitoring
• SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host
• The Tarantula Nebula as a template for extragalactic star forming regions from VLT/MUSE and HST/STIS
• The Properties of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants
• SNR G292.0+1.8: A Remnant of a Low-Mass Progenitor Stripped-Envelope Supernova
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• Characterizing the Post-Red Supergiant binary system AFGL 4106 and its complex nebula with SPHERE/VLT
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• Quantifying Systematic Age Discrepancies in Very Young Star Clusters
• EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
• Formation of massive multiple-star systems: early migration and mergers
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• Long Term X-Ray Spectral Variation of the Wolf-Rayet Binary WR 102-1 in the Galactic bulge: evidence for wind distortion in the binary
• An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons
• Dynamical double black holes and their host cluster properties
• Stellar multiplicity and stellar rotation: Insights from APOGEE
• Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• New mass estimates for massive binary systems: a probabilistic approach using polarimetric radiative transfer
• The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
• A Kinematically Cold Structure of Candidate Young OB Stars Toward The Anticenter
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images
• Stellar Multiplicity in Open Clusters: Investigating Binary Fractions and Their Relationship with Cluster Properties
• Investigation of projected rotational velocities of Be-type stars in LAMOST DR7
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• Chemical fingerprints of binary mass transfer in massive stars
• Spectral Dataset of Stripped-Envelope Supernovae from the Tsinghua Supernova Group
• Formation of black holes from He stars
• Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging