Evolution of binary stars and the effect of tides on binary populations

Abstract

We present a rapid binary evolution algorithm that enables modelling of even the most complex binary systems. In addition to all aspects of single star evolution, features such as mass transfer, mass accretion, common-envelope evolution, collisions, supernova kicks and angular momentum loss mechanisms are included. In particular, circularization and synchronization of the orbit by tidal interactions are calculated for convective, radiative and degenerate damping mechanisms. We use this algorithm to study the formation and evolution of various binary systems. We also investigate the effect that tidal friction has on the outcome of binary evolution. Using the rapid binary code, we generate a series of large binary populations and evaluate the formation rate of interesting individual species and events. By comparing the results for populations with and without tidal friction we quantify the hitherto ignored systematic effect of tides and show that modelling of tidal evolution in binary systems is necessary in order to draw accurate conclusions from population synthesis work. Tidal synchronism is important but because orbits generally circularize before Roche-lobe overflow the outcome of the interactions of systems with the same semi-latus rectum is almost independent of eccentricity. It is not necessary to include a distribution of eccentricities in population synthesis of interacting binaries, however, the initial separations should be distributed according to the observed distribution of semi-latera recta rather than periods or semi-major axes.

36 pages, 12 figures, to be published in the Monthly Notices of the Royal Astronomical Society

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• How Many CVs are Crossing the Period Gap? A Test for the Disruption of Magnetic Braking
• The birth properties of Galactic millisecond radio pulsars
• Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
• The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
• WD 1856 b: a close giant planet around a white dwarf that could have survived a common-envelope phase
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- IV. cataclysmic variables -- properties of bright and faint populations
• MOCCA Survey Database I: Dissolution of tidally filling star clusters harbouring BH subsystems
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• No cataclysmic variables missing: higher merger rate brings into agreement observed and predicted space densities
• Population Synthesis for Symbiotic X-ray Binaries
• Post-common envelope binaries from SDSS - XVI. Long orbital period systems and the energy budget of CE evolution
• Gaia May Detect Hundreds of Well-characterised Stellar Black Holes
• An analytic model for mass transfer in binaries with arbitrary eccentricity, with applications to triple-star systems
• The dynamical formation of LMXBs in dense stellar environments: globular clusters and the inner bulge of M31
• A common-envelope wind model for Type Ia supernovae (I): binary evolution and birth rate
• Dynamical Evolution of Multiple-Population Globular Clusters
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Precessional instability in binary black holes with aligned spins
• X-Ray Binary Populations: The Luminosity Function of NGC1569
• Population synthesis of wide binary millisecond pulsars
• The double-degenerate model for the progenitors of type Ia supernovae
• Can Neutron-Star Mergers Explain the r-process Enrichment in Globular Clusters?
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation III: dissecting black hole dynamics
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations
• Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah challenge Newtonian gravitation
• Binary population synthesis models for core-collapse gamma-ray burst progenitors
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• A Population of Ultraluminous X-ray Sources with An Accreting Neutron Star
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Transients from ONe White-Dwarf - Neutron-Star/Black-Hole Mergers
• Electron Capture Supernovae From Close Binary Systems
• Main-sequence progenitor configurations of the NN Ser candidate circumbinary planetary system are dynamically unstable
• Evolution of stellar collision products in open clusters. II. A grid of low-mass collisions
• Wind-accreting Symbiotic X-ray Binaries
• Gravitational signatures of a non--commutative stable black hole
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Population Synthesis of Black Hole Binaries with Normal-Star Companions: I. Detached Systems
• Core radius evolution of star clusters
• On Rejuvenation in Massive Binary Systems
• On equilibrium tides in fully convective planets and stars
• Towards an N-body Model for the Globular Cluster M4
• Do R Coronae Borealis Stars Form from Double White Dwarf Mergers?
• Supercritical accretion of stellar-mass compact objects in active galactic nuclei
• On the Formation of Ultraluminous X-ray Sources with Neutron Star Accretors: the Case of M82 X-2
• In Search of the Thermal Eccentricity Distribution
• Supernova Kicks and Misaligned Be Star Binaries
• The Formation of EL CVn-type Binaries
• Observed binary populations reflect the Galactic history. Explaining the orbital period-mass ratio relation in wide hot subdwarf binaries
• A new Monte Carlo method for dynamical evolution of non-spherical stellar systems
• SPISEA: A Python-Based Simple Stellar Population Synthesis Code for Star Clusters
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• Origin of the early-type R stars: a binary-merger solution to a century-old problem?
• The occurrence of Binary Evolution Pulsators in the classical instability strip of RR Lyrae and Cepheid variables
• Population synthesis of helium white dwarf--red giant star mergers and the formation of lithium-rich giants and carbon stars
• Predicting Stellar-Mass Black Hole Populations in Globular Clusters
• The host galaxies of double compact objects merging in the local Universe
• Chaotic dynamics of wide triples induced by galactic tides: a novel channel for producing compact binaries, mergers, and collisions
• Planetary nebulae after common-envelope phases initiated by low-mass red giants
• Population synthesis of Galactic subdwarf B stars
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• Binary coalescence from case A evolution -- mergers and blue stragglers
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Transition of the Stellar Initial Mass Function Explored with Binary Population Synthesis
• The Contributions of Interactive Binary Stars to Double Main Sequence Turn-Offs and Dual Red Clump of Intermediate-Age Star Clusters
• A new age determination Gamma^2 Velorum from binary stellar evolution models
• Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
• Detection of a $\sim$100,000 M${}_{\odot }$ black hole in M31's most massive globular cluster: A tidally stripped nucleus
• New low mass ratio contact binaries in the Catalina Sky Survey
• The birth rate of SNe Ia from hybrid CONe white dwarfs
• A spectroscopic investigation of the O-type star population in four Cygnus OB associations. I. Determination of the binary fraction
• Consequences of Dynamical Disruption and Mass Segregation for the Binary Frequencies of Star Clusters
• Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• How to Make a Singleton sdB Star via Accelerated Stellar Evolution
• The helium star donor channel for the progenitors of type Ia supernovae with different metallicities
• The hybrid CONe WD + He star scenario for the progenitors of type Ia supernovae
• Low Mass X-ray Binaries and Metallicity Dependence: Story of Failures
• Double Compact Objects as Low-frequency Gravitational Wave Sources
• Population Synthesis of Black Hole X-Ray Binaries
• GRB 211211A: a Neutron Star$-$White Dwarf Merger?
• Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties
• Stellar Escape from Globular Clusters. I. Escape Mechanisms and Properties at Ejection
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• Rejuvenated accretors have less bound envelopes: Impact of Roche lobe overflow on subsequent common envelope events
• Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters
• Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
• Ultra-compact X-ray binaries with He star companions
• Combined Effects of Binaries and Stellar Rotation on the Color-Magnitude Diagrams of Intermediate-Age Star Clusters
• Anisotropic winds in Wolf-Rayet binary identify potential gamma-ray burst progenitor
• Mass Transfer in Binary Stars using SPH. II. Eccentric Binaries
• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
• Dynamics of binary black holes in low-mass young star clusters
• Planetary systems in a star cluster I: the Solar system scenario
• Population synthesis in astrophysics
• On the Spin Period Distribution in Be/X-ray Binaries
• Effects of chemical composition and thermohaline mixing on the accreting components for low--mass close binaries: application to blue stragglers
• The population of white dwarf-main sequence binaries in the SDSS DR 12
• Simulations predict intermediate-mass black hole formation in globular clusters
• Double Neutron Star Formation: Merger Times, Systemic Velocities, and Travel Distances
• Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
• On the Origin of Sub-Subgiant Stars II: Binary Mass Transfer, Envelope Stripping, and Magnetic Activity
• The White Dwarf Binary Pathways Survey IV: Three close white dwarf binaries with G-type secondary stars
• Double neutron star mergers from hierarchical triple-star systems
• On the Chandra X-ray Sources in the Galactic Center
• The velocity dispersion and mass function of the outer halo globular cluster Palomar 4
• MODEST-1: Integrating Stellar Evolution and Stellar Dynamics
• Dynamical evolution of Population III stellar systems and the resulting binary statistics
• SALT reveals the barium central star of the planetary nebula Hen 2-39
• A Census of Blue Stragglers in Gaia DR2 Open Clusters as a Test of Population Synthesis and Mass Transfer Physics
• On the evolution of rotating accreting white dwarfs and type Ia supernovae
• Tidal capture formation of Low Mass X-Ray Binaries from wide binaries in the field
• Impact of binary interactions on the diffuse supernova neutrino background
• Spin it as you like: the (lack of a) measurement of the spin tilt distribution with LIGO-Virgo-KAGRA binary black holes
• Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
• A prescription and fast code for the long-term evolution of star clusters - III. Unequal masses and stellar evolution
• Evolutionary Population Synthesis for Binary Stellar Population at High Spectral Resolution: Integrated Spectral Energy Distributions and Absorption-feature Indices
• Helium star evolutionary channel to super-Chandrasekhar mass type Ia supernovae
• Nebular emission from young stellar populations including binary stars
• Molecular emission from GG Car's circumbinary disk
• Population Synthesis of Galactic Be-star Binaries with A Helium-star Companion
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• Direct $N$-body simulations of globular clusters - II. Palomar 4
• Astrophysical false positives in direct imaging for exoplanets: a white dwarf close to a rejuvenated star
• Evolution models of helium white dwarf--main sequence star merger remnants
• N-body models of globular clusters: metallicity, half-light radii and mass-to-light ratios
• Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters
• White dwarf masses in cataclysmic variables
• Mass Evaporation Rate of Globular Clusters in a Strong Tidal Field
• On the Formation of Galactic Black Hole Low-Mass X-ray Binaries
• Monte Carlo simulations of star clusters -- III. A million body star cluster
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• The orbit and stellar masses of the archetype colliding-wind binary WR 140
• Population synthesis of accreting white dwarfs: II. X-ray and UV emission
• Dynamical Tides Reexpressed
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• Dust Formation in the Ejecta of Common Envelope Systems
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• The study of eleven contact binaries with mass ratios less than 0.1
• Black hole spins in coalescing binary black holes
• On the true shape of the upper end of the stellar initial mass function: The case of R136
• Evidence for the evolution of black hole mass function with redshift
• Population Synthesis of Hot Subdwarfs: A Parameter Study
• Transient Low-Mass X-Ray Binary Populations in Elliptical Galaxies NGC 3379 and NGC 4278
• 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
• The violent white dwarf merger scenario for the progenitors of type Ia supernovae
• Populating the Galaxy with pulsars -- II. Galactic dynamics
• RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich
• SNe Kicks in Hierarchical Triple Systems
• Constraints on single-degenerate Chandrasekhar mass progenitors of Type Iax supernovae
• Gravitational traces of bumblebee gravity in metric-affine formalism
• Initial Populations of Black Holes in Star Clusters
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- I. cataclysmic variables -- present-day population
• Comparing Compact Object Distributions from Mass- and Presupernova Core Structure-based Prescriptions
• Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae
• From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers
• Gaia Reveals Evidence for Merged White Dwarfs
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• An extended Pal 5 stream in Gaia DR2
• On the rates of type Ia supernovae originating from white dwarf collisions in quadruple star systems
• Fundamental Properties of Co-Moving Stars observed by $Gaia$
• Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESA
• The Initial Mass Function of the Inner Galaxy Measured From OGLE-III Microlensing Timescales
• Gravitational Wave Background of Neutron Star-White Dwarf Binaries
• Non-interacting black hole binaries with Gaia and LAMOST
• Do the majority of stars form as gravitationally unbound?
• Common Envelope Mergers: A Possible Channel for Forming Single sdB Stars
• Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars
• Observability of inflated companion stars after supernovae in massive binaries
• Evolution of massive stellar triples and implications for compact object binary formation
• Nonconservative Mass Transfer in Massive Binaries and the Formation of Wolf-Rayet+O Binaries
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• Disk Material Inflates Gaia RUWE Values in Single Stars
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• Understanding the orbital periods of CEMP-s stars
• Landscape of stellar-mass black-hole spectroscopy with third-generation gravitational-wave detectors
• Constraining Mass Transfer Histories of Blue Straggler Stars with COS Spectroscopy of White Dwarf Companions
• A dynamical gravitational wave source in a dense cluster
• Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events
• The host galaxies of double compact objects across cosmic time
• The evolution of the self-lensing binary KOI-3278: evidence of extra energy sources during CE evolution
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• The state of globular clusters at birth: emergence from the gas-embedded phase
• Genesis of magnetic fields in isolated white dwarfs
• Magnetars from Neutron Star--White Dwarf Mergers: Application to Fast Radio Bursts
• Roche-lobe overflow systems powered by black holes in young star clusters: the importance of dynamical exchanges
• A potential mass-gap black hole in a wide binary with a circular orbit
• WIYN Open Cluster Study. LXXVII. Radial-Velocity Measurements and Spectroscopic Binary Orbits in the Open Cluster NGC 7789
• Return of the TEDI: revisiting the Triple Evolution Dynamical Instability channel in triple stars
• Analysis of a regular black hole in Verlinde's gravity
• The impact of white dwarf natal kicks and stellar flybys on the rates of Type Ia supernovae in triple-star systems
• Constraints on the Binary Companion to the SN Ic 1994I Progenitor
• Exploring compact binary merger host galaxies and environments with $\mathrm{zELDA}$
• A formation scenario for the triple pulsar PSR J0337+1715: breaking a binary system inside a common envelope
• Evolution and CNO yields of Z=10^-5 stars and possible effects on CEMP production
• Early-type Eclipsing Binaries with Intermediate Orbital Periods
• Pre-explosion companion stars in Type Iax supernovae
• The influence of stellar-dynamical ejections and collisions on the relation between the maximum-star and star-cluster-mass
• Evolution of the number of accreting white dwarfs with shell nuclear burning and of occurrence rate of SN Ia
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history
• Tidal-locking-induced stellar rotation dichotomy in the open cluster NGC 2287?
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• Eclipsing binaries in extrasolar planet transit surveys: the case of SuperWASP
• Compact Object Modeling in the Globular Cluster 47 Tucanae
• A statistical view on stable and unstable Roche lobe overflow of a tertiary star onto the inner binary in triple systems
• On the Link Between Energy Equipartition and Radial Variation in the Stellar Mass Function of Star Clusters
• Dynamical Formation of Cataclysmic Variables in Globular Clusters
• The origin of single low-mass WDs: another problem that consequential angular momentum loss in CVs might solve
• The Gaia-ESO Survey: detection and characterization of single line spectroscopic binaries
• The eccentric behaviour of windy binary stars
• On the Origin of Sub-subgiant Stars. III. Formation Frequencies
• Effects of non-commutative geometry on black hole properties
• A population synthesis fitting of the $Gaia$ resolved white dwarf binary population within 100 pc
• Galactic Model Parameters and Space Density of Cataclysmic Variables in Gaia Era: New Constraints to Population Models
• First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics
• A systematic study of effects of stellar rotation, age spread and binaries on color-magnitude diagrams with extended main-sequence turn-offs
• From Canonical to Enhanced Extra Mixing in Low-Mass Red Giants: Tidally Locked Binaries
• Early ultraviolet signatures from the interaction of Type Ia supernova ejecta with a stellar companion
• Black hole - black hole total merger mass and the origin of LIGO/Virgo sources
• Some constraints on the lower mass limit for double-degenerate progenitors of Type Ia supernovae
• Binary evolution along the Red Giant Branch with BINSTAR: The barium star perspective
• Prospects for detecting asteroseismic binaries in Kepler data
• Disc-binary interactions in depleted post-AGB binaries
• Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study
• Binary companions of nearby supernova remnants found with Gaia
• The first pre-supersoft X-ray binary
• Massive black hole assembly in nuclear star clusters
• The Detection of Dust around NN Ser
• HV2112, a Thorne-Zytkow Object or a Super Asymptotic Giant Branch Star
• On the role of supernova kicks in the formation of Galactic double neutron star systems
• Occultation Searches for Kuiper Belt Objects
• How binary interactions affect spectral stellar population synthesis
• An Isochrone Database and a Rapid Model for Stellar Population Synthesis
• Massive binary black holes from Population II and III stars
• Companion stars of Type Ia supernovae and single low-mass white dwarfs
• Very massive stars in not so massive clusters
• Dispersion and Rotation Measures from the Ejecta of Compact Binary Mergers: Clue to the Progenitors of Fast Radio Bursts
• Massive binary star mergers in galactic nuclei: implications for blue stragglers, binary S-stars and gravitational waves
• Black Hole/Pulsar Binaries in the Galaxy
• Evolutionary models of short-period soft X-ray transients: comparison with observations
• An incisive look at the symbiotic star SS Leporis -- Milli-arcsecond imaging with PIONIER/VLTI
• Monte Carlo population synthesis of post-common-envelope white dwarf binaries and type Ia supernova rate
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• The impact of primordial binary on the dynamical evolution of intermediate massive star clusters
• Circumbinary discs for stellar population models
• Modeling X-ray binary evolution in normal galaxies: Insights from SINGS
• FROST: a momentum-conserving CUDA implementation of a hierarchical fourth-order forward symplectic integrator
• Globular cluster formation histories, masses and radii inferred from gravitational waves
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• Stellar Core-Merger-Induced Collapse: New Formation Pathways for Black Holes, Thorne-$\dot{\mathrm{Z}}$ytkow objects, Magnetars and Superluminous Supernovae
• Constraints on compact binary merger evolution from spin-orbit misalignment in gravitational-wave observations
• Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all
• On the population III binary black hole mergers beyond the pair-instability mass gap
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Prospects of gravitational-waves detections from common-envelope evolution with LISA
• V605 Aquilae: a born again star, a nova or both?
• Modelling nova populations in galaxies
• The formation of single neutron-stars from double white-dwarf mergers via accretion-induced collapse
• Low-mass X-ray binaries from black-hole retaining globular clusters
• The occurrence of classical Cepheids in binary systems
• On the Common Envelope Efficiency
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• A tale of caution: the tails of NGC 752 are much longer than claimed
• Powerful CMD: A Tool for Colour-Magnitude Diagram Studies
• Dissecting the Gaia HR diagram within 200 pc
• Evolution of star cluster systems in isolated galaxies: first results from direct $N$-body simulations
• Gaia's Detectability of Black Hole-Main Sequence Star Binaries Formed in Open Clusters
• Possible smoking-gun evidence for initial mass segregation in re-virialized post-gas expulsion globular clusters
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Supernova Kicks and Dynamics of Compact Remnants in the Galactic Centre
• The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
• The Role of "Black Hole Burning" in the Evolution of Dense Star Clusters
• The connection between merging double compact objects and the Ultraluminous X-ray Sources
• Do SN 2002cx-like and SN Ia-CSM objects share the same origin?
• The dynamical origin of multiple populations in intermediate-age clusters in the Magellanic Clouds
• A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
• Features of Gaia DR3 Spectroscopic Binaries I. Tidal circularization of Main-Sequence Stars
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Stellar Spins in the Open Cluster NGC 2516
• Period bouncers as detached magnetic cataclysmic variables
• MOCCA-SURVEY Database I: Is NGC 6535 a Dark Star Cluster Harboring an IMBH?
• Binary stars and the UVX in early type galaxies
• Binary black hole mergers from young massive clusters in the pair-instability supernova mass gap
• Stars on the run: escaping from stellar clusters
• Observational signatures of past mass-exchange episodes in massive binaries: The case of HD 149 404
• The gravitational-wave signal generated by a galactic population of double neutron-star binaries
• Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
• Precise radial velocities of giant stars IX. HD 59686 Ab: a massive circumstellar planet orbiting a giant star in a ~13.6 au eccentric binary system
• The single-degenerate model for the progenitors of accretion-induced collapse events
• Matching Globular Cluster Models to Observations
• Evolution and final fate of massive post-common-envelope binaries
• HE 0430-2457: a post merger extremely low-mass pre-white dwarf in a wide binary posing as an extreme horizontal branch star
• The progenitors of type Ia supernovae in the semidetached binaries with red giant donors
• Radial Variation in the Stellar Mass Functions of Star Clusters
• Spin Angular Momentum Evolution of the Long Period Algols
• Population Synthesis of Common Envelope Mergers: I. Giant Stars with Stellar or Substellar Companions
• Are white dwarf magnetic fields in close binaries generated during common-envelope evolution?
• The coupled effect of tides and stellar winds on the evolution of compact binaries
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• The active W UMa type binary star V781 Tau revisited
• The blue straggler V106 in NGC6791: A prototype progenitor of old single giants masquerading as young
• Constraining Compact Object Formation with 2M0521
• The Value-Added Catalog of ASAS-SN Eclipsing Binaries: Parameters of Thirty Thousand Detached Systems
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• The effect of intermediate mass close binaries on the chemical evolution of Globular Clusters
• The Orbital Nature of 81 Ellipsoidal Red Giant Binaries in the Large Magellanic Cloud
• Dynamical formation of the GW190814 merger
• Simulating the Legacy Survey of Space and Time stellar content with TRILEGAL
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo
• Phase-dependent study of near-infrared disk emission lines in LB-1
• Tidal Interactions in Post Common-Envelope sdB Binaries
• Exploring compact binary populations with the Einstein Telescope
• Dynamical modelling of globular clusters: challenges for the robust determination of IMBH candidates
• Demographics of triple systems in dense star clusters
• Evaluating the impact of binary parameter uncertainty on stellar population properties
• The true stellar parameters of the Kepler target list
• Modelling Collision Products of Triple-Star Mergers
• Predictions of a simple parametric model of hierarchical black hole mergers
• The Brightest Point X-Ray Sources in Elliptical Galaxies and the Mass Spectrum of Accreting Black Holes
• Blue Large-Amplitude Pulsators: the Possible Surviving Companions of Type Ia Supernovae
• Forming merging double compact objects with stable mass transfer
• BIFROST: simulating compact subsystems in star clusters using a hierarchical fourth-order forward symplectic integrator code
• Binary parameters from astrometric and spectroscopic errors--candidate hierarchical triples and massive dark companions in Gaia DR3
• What binary systems are the most likely sources for periodically repeating FRBs?
• MOCCA: Dynamics and evolution of binary stars of multiple stellar populations in tidally filling and underfilling globular star clusters
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• Mining for Candidates of Galactic Stellar-mass Black Hole Binaries with LAMOST
• Companion-driven evolution of massive stellar binaries
• Eclipse Timings of the LMXB XTE J1710-281: Orbital Period Glitches
• Two decades of optical timing of the shortest-period binary star system HM Cancri
• The Black Hole Mass Function Across Cosmic Times I. Stellar Black Holes and Light Seed Distribution
• Effects of Irradiation on the Evolution of Ultra-compact X-ray Binaries
• Population synthesis on high-mass X-ray binaries: prospects and constraints from the universal X-ray luminosity function
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• A fast spinning magnetic white dwarf in the double-degenerate, super-Chandrasekhar system NLTT 12758
• Population III X-ray Binaries and their Impact on the Early Universe
• The impact of metallicity-dependent mass loss versus dynamical heating on the early evolution of star clusters
• Explanation of a special color-magnitude diagram of star cluster NGC 1651 from different models
• Theoretical orbital period distributions of cataclysmic variables above the period gap: effects of circumbinary disks
• Deep ACS Imaging in the Globular Cluster NGC6397: Dynamical Models
• Revisiting binary stars in population synthesis models
• A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• The impact of massive stars and black holes on the fate of open star clusters and their tidal streams
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• The Nature of the Faint Chandra X-ray Sources in the Galactic Centre
• Formation and Evolution of Ultraluminous X-ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems
• A population synthesis study on the faint X-ray sources in the Galactic center region
• A close-in giant planet escapes engulfment by its star
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• The detached-binary channel for the formation of contact binaries
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- III. Cataclysmic variables -- Implications of model assumptions
• Implications of a Simpson-Visser solution in Verlinde's framework
• Formation and Evolution of Galactic Intermediate/Low-Mass X-ray Binaries
• A pair of CO + He white dwarfs as the progenitor of 2005E-like supernovae?
• Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation
• The Tarantula Massive Binary Monitoring project: II. A first SB2 orbital and spectroscopic analysis for the Wolf-Rayet binary R145
• Exploring the impact of IMF and binary parameter stochasticity with a binary population synthesis code
• On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
• Modeling contact binaries, II. The effect of energy transfer
• Detectablity of Black Hole Binaries with Gaia: Dependence on Binary Evolution Models
• The formation of long-period eccentric binaries with a helium white dwarf
• Binary black hole mergers from merged stars in the Galactic field
• The Blue Stragglers of the Old Open Cluster NGC 188
• Impact of initial mass functions on the dynamical channel of gravitational wave sources
• On the existence of brown dwarfs more massive than the hydrogen burning limit
• Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion
• Influence of a mass transfer stability criterion on double white dwarf populations
• The effect of primordial mass segregation on the size scale of globular clusters
• The frequency of Kozai-Lidov disc oscillation driven giant outbursts in Be/X-ray binaries
• Exploration of the $\ps-\pb$ Relation for Wind-Fed X-Ray Pulsars
• On the serendipitous discovery of a Li-rich giant in the globular cluster NGC 362
• Carbon Rich Extremely Metal Poor Stars: Signatures of Population-III AGB stars in Binary Systems
• The birth rate of supernovae from double-degenerate and core-degenerate systems
• Revisiting Common Envelope Evolution -- A New Semi-Analytic Model for N-body and Population Synthesis Codes
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• Core radii and common-envelope evolution
• Golden galactic binaries for LISA: mass-transferring white dwarf black hole binaries
• Spatial distribution of luminous X-ray binaries in spiral galaxies
• Mock Observations of Blue Stragglers in Globular Cluster Models
• Modelling the Observed Stellar Mass Function and its Radial Variation in Galactic Globular Clusters
• Triple evolution: an important channel in the formation of type Ia supernovae
• Stellar Population Diagnostics of the Massive Star Binary Fraction
• White-dwarf+main-sequence binaries identified from the tenth data release of Solan Digital Sky Survey
• Is there a Size Difference between Red and Blue Globular Clusters?
• The Lifetimes of Star Clusters Born with a Top-heavy IMF
• Finding Black Holes with Black Boxes -- Using Machine Learning to Identify Globular Clusters with Black Hole Subsystems
• Exploring the borderline between stable mass transfer and mergers in close binary evolution
• On the detection of pre-low-mass X-ray binaries
• The CO White Dwarf + Intermediate Mass/Massive Star Binary Evolution: Possible Merger Origins for Peculiar Type Ia and II Supernovae
• Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius--mass relation of embedded clusters
• From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
• A nova re-accretion model for J-type carbon stars
• Applying the metallicity-dependent binary fraction to double white dwarf formation: Implications for LISA
• Magnetic dynamos in white dwarfs -- I. Explaining the dearth of bright intermediate polars in globular clusters
• Rapid orbital decay in detached binaries: evidence for circumbinary disks
• Critical Mass Transfer in Double-Degenerate Type Ia Supernovae
• The White Dwarf Binary Pathways Survey -- IX. Three long period white dwarf plus subgiant binaries
• How important is secular evolution for black hole and neutron star mergers in 2+2 and 3+1 quadruple-star systems?
• The non-explosive stellar merging origin of the ultra-massive carbon-rich white dwarfs
• The birth rate of subluminous and overluminous type Ia supernovae
• On the origin of black hole spin in high-mass black hole binaries: Cygnus X-1
• The Magnetized White Dwarf + Helium star Binary Evolution with Accretion-induced Collapse
• Detection of satellite remnants in the Galactic Halo with Gaia III. Detection limits for Ultra Faint Dwarf Galaxies
• The black hole retention fraction in star clusters
• Barium Surface Abundances of Blue Stragglers in the Open Cluster NGC 6819
• Tidal Dissipation Impact on the Eccentric Onset of Common Envelope Phases in Massive Binary Star Systems
• The spin, expansion and contraction of open star clusters
• Observable fractions of core-collapse supernova light curves brightened by binary companions
• LISA sources from young massive and open stellar clusters
• Evidence for conservative mass transfer in the classical Algol system $\delta$ Librae from its surface carbon-to-nitrogen abundance ratio
• Binary fractions of G and K dwarf stars based on the Gaia EDR3 and LAMOST DR5: impacts of the chemical abundances
• Birthrates and delay times of Type Ia supernovae
• Formation and Destiny of White Dwarf and Be Star Binaries
• A young contracting white dwarf in the peculiar binary HD 49798/RX J0648.0--4418?
• MOCCA code for star cluster simulations - VI. Bimodal spatial distribution of blue stragglers
• A prescription and fast code for the long-term evolution of star clusters - II. Unbalanced and core evolution
• Population synthesis of accreting white dwarfs: Rates and evolutionary pathways of H and He novae
• The critical binary star separation for a planetary system origin of white dwarf pollution
• Oxygen-neon rich merger during common envelope evolution
• Hypercritical Accretion for Black Hole High Spin in Cygnus X-1
• Tracing CNO exposed layers in the Algol-type binary system u Her
• Hydrodynamic Winds From Twin-Star Binaries
• On the absence of symbiotic stars in globular clusters
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• The first photometric and spectroscopic analysis of the extremely low mass ratio contact binary NSVS 5029961
• Convection and rotation boosted prescription of magnetic braking: application to the formation of extremely low-mass white dwarfs
• New insights in the origin and evolution of the old, metal-rich open cluster NGC 6791
• Open star clusters and their asymmetrical tidal tails
• Formation of long-period post-common-envelope binaries I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence stars
• Companion Stars of Type Ia supernovae with different metallicities
• Potential Importance of Binary Evolution in UV-Optical Spectral Fitting of Early-Type Galaxies
• A Population of Neutron Star Ultraluminous X-ray Sources with A Helium Star Companion
• The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: spectroscopy, orbital analysis, formation, and evolution
• Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters
• Forming Hot Subluminous Stars from Hierarchical Triples -- I. The Role of an Outer Tertiary on Formation Channels
• The effects of the overshooting of the convective core on main-sequence turnoffs of young- and intermediate-age star clusters
• Contribution of primordial binary evolution to the two blue-straggler sequences in globular cluster M30
• Runaway and Hypervelocity Stars from Compact Object Encounters in Globular Clusters
• TIC 308396022: a $\delta$ Scuti--$\gamma$ Doradus hybrid with large-amplitude radial fundamental mode and regular g-mode period spacing
• The boring history of Gaia BH3 from isolated binary evolution
• Towards Multiple-Star Population Synthesis
• MOCCA-SURVEY Database II -- Properties of Intermediate Mass Black Holes escaping from star clusters
• The impact of metallicity on nova populations
• Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
• An ancient double degenerate merger in the Milky Way halo
• The core-degenerate scenario for the progenitors of type Ia supernovae
• Merging of a CO WD and a He-rich white dwarf to produce a type Ia supernovae
• The most metal-rich asymptotic giant branch stars
• Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
• Supernova Kicks and Misaligned Microquasars
• A Comparison of Rotating and Binary Stellar Evolution Models: Effects on Massive Star Populations
• Black Holes In Young Stellar Clusters
• Assessing the complexity of orbital parameters after asymmetric kick in binary pulsars
• Population Synthesis of Millisecond X-ray Pulsars
• Little Red Dots Are Nurseries of Massive Black Holes
• A Common Envelope Binary Star Origin of Long Gamma-ray Bursts
• A Catalog of Short Period Spectroscopic and Eclipsing Binaries Identified from the LAMOST & PTF Surveys
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes
• Two paths of cluster evolution: global expansion versus core collapse
• The contribution of dissolving star clusters to the population of ultra-faint objects in the outer halo of the Milky Way
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- II. Cataclysmic variables -- progenitors and population at birth
• A Gemini Snapshot Survey for Double Degenerates
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. I. HD 224355
• Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity
• A Triple Star Origin For T Pyx and Other Short-Period Recurrent Novae
• Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
• The role of binarity and stellar rotation in the split main sequence of NGC 2422
• Mergers of neutron stars and black holes with cores of giant stars: a population synthesis study
• A pulsar-helium star compact binary system formed by common envelope evolution
• A Non-Commutative Kalb-Ramond Black Hole
• 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
• A Triple Scenario for the Formation of Wide Black Hole Binaries Such As Gaia BH1
• Stellar-mass black holes in the Hyades star cluster?
• Post-AGB discs from common-envelope evolution
• Observational signatures of past mass-exchange episodes in massive binaries: The case of LSS 3074
• He star evolutionary channel to intermediate-mass binary pulsar PSR J1802-2124
• On the displacement of X-ray binaries from star clusters in star-burst galaxies
• A Fallback Disk Accretion-Involved Formation Channel to PSR J1903+0327
• Population synthesis of ultraluminous X-ray sources with magnetised neutron stars
• Star Cluster Formation from Turbulent Clumps. III. Across the mass spectrum
• The Signature of Single-Degenerate Accretion Induced Collapse
• A Monte Carlo study of early gas expulsion and evolution of star clusters: new simulations with the MOCCA code in the AMUSE framework
• TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars
• Gravitational-wave radiation from double compact objects with eLISA in the Galaxy
• Rapidly rotating neutron star progenitors
• Rates and delay times of Type Ia supernovae in the helium-enriched main-sequence donor scenario
• A strange star scenario for the formation of isolated millisecond pulsars
• A Survey for High-Mass Eclipsing Binaries
• Post-merger evolution of double helium white dwarfs and distribution of helium-rich hot subdwarfs
• The formation of subdwarf A-type stars
• Efficiency of black hole formation via collisions in stellar systems: An analysis of data from simulations and observations
• Properties of an axisymmetric Lorentzian non-commutative black hole
• A New Hybrid Technique for Modeling Dense Star Clusters
• MOCCA code for star cluster simulations - V. Initial globular cluster conditions influence on blue stragglers
• Lower-mass-gap Black Holes in Dense Star Clusters
• Habitability properties of circumbinary planets
• Stellar Triples as a Source for Ba Stars
• Automatic classification of eclipsing binary stars using deep learning methods
• The influence of star formation history on the gravitational wave signal from close double degenerates in the thin disc
• Star Cluster Formation from Turbulent Clumps. I. The Fast Formation Limit
• Binary black hole mergers from Population III star clusters
• Integrated spectral energy distributions of binary star composite stellar populations
• Eclipsing binary statistics - theory and observation
• Tidal Wave Breaking in the Eccentric Lead-In to Mass Transfer and Common Envelope Phases
• Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars
• Formation and Evolution of Accreting Compact Objects
• Minimum Orbital Period of Pre-Cataclysmic Variables
• Understanding the progenitor formation galaxies of merging binary black holes
• Star formation history, double degenerates and type Ia supernovae in the thin disc
• Non-commutativity in Hayward spacetime
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• Targeted modeling of GW150914's binary black hole source with dart_board
• Wandering off the centre: a characterization of the random motion of intermediate-mass black holes in star clusters
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• The dynamical mass and evolutionary status of the type-II Cepheid in the eclipsing binary system OGLE-LMC-T2CEP-211 with a double-ring disk
• The envelope mass of red giant donors in Type Ia supernova progenitors
• Towards an understanding of long gamma-ray burst environments through circumstellar medium population synthesis predictions
• On the role of reduced wind mass-loss rate in enabling exoplanets to shape planetary nebulae
• The OATMEAL Survey. I. Low Stellar Obliquity in the Transiting Brown Dwarf System GPX-1
• Unexpected Short-Period Variability in Dwarf Carbon Stars from the Zwicky Transient Facility
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• Impact of binary interaction on the evolution of blue supergiants
• Radiation fields by intermediate-age stellar populations with binaries as ionizing sources of H II regions
• Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
• The mass distribution of stars stripped in binaries: The effect of metallicity
• Accretion disks in Algols: progenitors and evolution
• The Binary Black Hole Merger Rate from Ultraluminous X-ray Source Progenitors
• Hot subdwarf B stars with neutron star components II: Binary population synthesis
• A spider timing model: accounting for quadrupole deformations and relativity in close pulsar binaries
• The galactic rate of second and third generation disc and planet formation
• Carbon-enhanced stars with short orbital and spin periods
• The formation of the magnetic symbiotic star FN Sgr
• Galactic orbital motions of star clusters: static versus semicosmological time-dependent Galactic potentials
• Binary population synthesis study on supersoft X-ray phase of single degenerate type Ia supernova progenitors
• Circumstellar properties of Type Ia supernovae from the helium star donor channel
• Possible Contribution of Magnetized White Dwarf Binaries to Type Ia Supernova Populations
• On the dynamical evolution of Cepheids in star clusters
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• The origin of the high-mass X-ray binary 4U 2206+54/BD +53 2790
• Unraveling the Formation History of the Black Hole X-ray Binary LMC X-3 from ZAMS to Present
• IGR J18293-1213 is an eclipsing Cataclysmic Variable
• Globular clusters as probes of dark matter cusp-core transformations
• The effects of stellar population synthesis on the distributions of the asteroseismic observables ν_max and Δν of red-clump stars
• Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• The long and the short of it: modelling double neutron star and collapsar Galactic dynamics
• Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• A new white dwarf companion to the $\Delta \mu$ star GJ 3346
• Low-mass X-ray Binaries with Strange Quark Stars
• Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?
• Magnesium-rich Ejecta in the SNR G284.3$-$1.8 Around the High-Mass Gamma-Ray Binary 1FGL J1018.6$-$5856
• Orbital Eccentricity and Spin-Orbit Misalignment Are Evidence that Neutron Star-Black Hole Mergers Form through Triple Star Evolution
• Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The eclipsing binary HD 185912
• New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
• The impact of binaries on the evolution of star clusters from turbulent molecular clouds
• Variation in the Stellar Mass Function Along Stellar Streams
• Red giant depletion in globular cluster cores
• The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles
• Probing the efficiency of tidal synchronization in outspiralling double white dwarf binaries with LISA
• Three Ultra-short Period Contact Eclipsing Binary Systems Mined from Massive Astronomical Surveys
• Spatial and Binary Parameter Distributions of Black Hole Binaries in the Milky Way Detectable with Gaia
• The interacting double white dwarf population with LISA; stochastic foreground and resolved sources
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• The Contribution of Chemical Abundances in Nova Ejecta to the Interstellar Medium
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Possible confirmation of the existence of ergoregion by the Kerr quasinormal mode in gravitational waves from Pop III massive black hole binary
• Populations of evolved massive binary stars in the Small Magellanic Cloud II: Predictions from rapid binary evolution
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• Planet formation in post-common-envelope binaries
• Constraining Intermediate-Mass Black Holes in Globular Clusters
• On the Rarity of X-Ray Binaries with Naked Helium Donors
• On the origin of the split main sequences of the young massive cluster NGC 1856
• The effect of metallicity on the delay-time distribution of type Ia supernova
• On the White Dwarf Mass Problem of Cataclysmic Variables
• B fields in OB stars (BOB): The magnetic triple stellar system HD 164492C in the Trifid nebula
• Probing the Survival of Planetary Systems in Globular Clusters with Tidal Disruption Events
• The Blue Lurker WOCS 14020: A Long-Period Post-Common-Envelope Binary in M67 Originating from a Merger in a Triple System
• Primordial mass segregation of star clusters with primordial binaries
• MOCCA Survey Database: Extra Galactic Globular Clusters. I. Method and first results
• The rate of iPTF 14gqr like ultra-stripped supernovae and binary evolution leading to double neutron star formation
• New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observations
• Convection physics and tidal synchronization of the subdwarf binary NY Virginis
• The White Dwarf Binary Pathways Survey III: contamination from hierarchical triples containing a white dwarf
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Energy equipartition in multiple-population globular clusters
• Energy Optimization in Binary Star Systems: Explanation for Equal Mass Members in Close Orbits
• MOCCA: Global properties of tidally filling and underfilling globular star clusters with multiple stellar populations
• IP Eri: A surprising long-period binary system hosting a He white dwarf
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Life after eruption VIII: The orbital periods of novae
• The binding energy produced within the framework of the accretion of millisecond pulsars
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Effects of the core-collapse supernova ejecta impact on a rapidly rotating massive companion star
• Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
• Cataclysmic Variables in Triples: Formation Models and New Discoveries
• Asymmetrical mass ejection from proto-white dwarfs and the formation of eccentric millisecond pulsar binaries
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
• He-star donor AM CVn stars and their progenitors as LISA sources
• On the distribution of stellar-sized black hole spins
• Great Balls of FIRE III: Modeling Black Hole Mergers from Massive Star Clusters in Simulations of Galaxies
• Novae: An Important Source of Lithium in the Galaxy
• Pre-mainsequence stellar evolution in N-body models
• Surrogate forward models for population inference on compact binary mergers
• GABE: Galaxy Assembly with Binary Evolution
• A possible giant planet orbiting the cataclysmic variable LX Ser
• Today a Duo, But Once a Trio? The Double White Dwarf HS 2220$+$2146 May Be A Post-Blue Straggler Binary
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• Scalable stellar evolution forecasting: Deep learning emulation vs. hierarchical nearest neighbor interpolation
• NGTS J214358.5-380102 -- NGTS discovery of the most eccentric known eclipsing M-Dwarf binary system
• Analytic approximations for massive close post-mass transfer binary systems
• Accretion of chemically fractionated material on a wide binary with a blue straggler
• Tidal Interaction in High Mass X-ray Binaries
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Spin evolution of neutron stars in wind-fed high mass X-ray binaries
• The possible existence of Pop III NS-BH binary and its detectability
• Galactic population of black holes in detached binaries with low-mass stripped helium stars: the case of LB-1 (LS~V+22~25)
• Testing the robustness of simulation-based gravitational-wave population inference
• The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
• Monte Carlo simulations of multiple populations in globular clusters: constraints on the initial size of the second generation from binary stars
• Type IIb supernovae by the grazing envelope evolution
• Testing tidal theory using Gaia binaries: the red giant branch
• Young stars in the Galactic Centre: a potential intermediate-mass star origin
• Mass-stream trajectories with non-synchronously rotating donors
• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• Uncertainties in the calibrations of star formation rate
• Dynamically Forming Extremely Low-Mass White Dwarf Binaries in Wide Orbits
• Fast rotating stars resulting from binary evolution will often appear to be single
• McScatter: a Simple Three-Body Scattering Package with Stellar Evolution
• Donors of Persistent Neutron-star Low-mass X-ray Binaries
• Mapping population synthesis event rates on model parameters II: Convergence and accuracy of multidimensional fits
• Dynamical detection of three triple stellar systems in open clusters
• Common Envelope Mechanisms: Constraints from the X-ray Luminosity Function of High Mass X-ray Binaries
• The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes
• WD + He star systems as the progenitors of Type Ia supernovae and their surviving companion stars
• Evolution models of helium white dwarf--main-sequence star merger remnants: the mass distribution of single low-mass white dwarfs
• The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure
• Long gamma ray burst rate in the binary merger progenitor model
• An Empirical Fit for Viscoelastic Simulations of Tertiary Tides
• Dynamical friction of a massive black hole in a turbulent gaseous medium
• Dynamical Tides in Eccentric Binaries Containing Massive Main-Sequence Stars: Analytical Expressions
• Binary Evolution: Roche Lobe Overflow and Blue Stragglers
• Can eccentric binary millisecond pulsars form by accretion induced collapse of white dwarfs?
• A population synthesis study of the Gaia 100 pc unresolved white dwarf-main sequence binary population
• Applications of Stellar Population Synthesis in the Distant Universe
• Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters
• LISC Catalog of Open Clusters.III. 83 Newly found Galactic disk open clusters using Gaia EDR3
• Gravitational wave spectral synthesis
• Astrometric mass measurement of compact companions in binary systems with Gaia
• MESA Models of the Evolutionary State of the Interacting Binary epsilon Aurigae
• COCOA Code for Creating Mock Observations of Star Cluster Models
• The mass distribution of stellar mergers: A new scenario for several FS CMa stars
• Formation of Sco X-1 induced by anomalous magnetic braking of Ap/Bp stars
• Fitting Formulae for the Effects of Binary Interactions on Lick Indices and Colours of Stellar Populations
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Generalised analytical results on $n$-ejection-collision orbits in the RTBP. Analysis of bifurcations
• Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product
• Discovery of two eclipsing X-ray binaries in M51
• A closer look at non-interacting He stars as a channel for producing the old population of Type Ia supernovae
• On the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth
• Can the Subsonic Accretion Model Explain the Spin Period Distribution of Wind-fed X-ray Pulsars?
• Statistics of Magrathea exoplanets beyond the Main Sequence. Simulating the long-term evolution of circumbinary giant planets with TRES
• Reconstructing post-common envelope white dwarf+main sequence binary histories through inverse population synthesis techniques
• On the large apparent black hole spin-orbit misalignment angle in GW200115
• Yunnan-III models for Evolutionary population synthesis
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• Accurate absolute parameters of the binary system V4089 Sgr
• A Be Star + He Star Binary as an Indicator of a Binary Mass Transfer Phase
• Orbital radius during the grazing envelope evolution
• DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations
• Searching for new observational signatures of the dynamical evolution of star clusters
• The contribution of X-ray binaries to the evolution of late-type galaxies: Evolutionary population synthesis simulations
• Unveiling the Binary Nature of NGC 2323
• Rethinking mass transfer: a unified semi-analytical framework for circular and eccentric binaries. I. Orbital evolution due to conservative mass transfer
• Millisecond Pulsars in Dense Star Clusters: Evolution, Scaling Relations, and the Galactic-Center Gamma-ray Excess
• Optical characterization and Radial velocity monitoring with Belgian and Indian Telescopes (ORBIT): the eclipsing binaries EPIC 211982753 and EPIC 211915147
• Binary imposters: Mergers in massive hierarchical triple stars
• The Ages of M31 Star Clusters: Spectral Energy Distribution Versus Color-Magnitude Diagram
• Ultraluminous X-ray sources with He star companions
• Astrophysics with the Laser Interferometer Space Antenna
• Young Blue Straggler Stars in the Galactic Field
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• MOCCA: Effects of pristine gas accretion and cluster migration on globular cluster evolution, global parameters, and multiple stellar populations
• X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
• Post-common envelope binary systems experiencing helium-shell driven stable mass transfer
• Thermal Timescale Mass Transfer Rates in Intermediate-Mass X-ray Binaries
• Phase-space mixing of multiple stellar populations in globular clusters
• Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors
• Investigating the UV-excess in star clusters with $N$-body simulations: predictions for future CSST observations
• Population Study of Astrophysical False Positive Detections in the Southern PLATO field
• The first photometric analysis of the totally eclipsing contact binary V811 Cep
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• The effects of UV photometry and binary interactions on photometric redshift and galaxy morphology
• The Initial Properties of Young Star Clusters in M83
• On the Formation of SS433
• Population and spectral synthesis: it doesn't work without binaries
• Simulating Kilonovae in the ΛCDM Universe
• Faint X-ray Binaries and Their Optical Counterparts in M31
• A super-Eddington wind scenario for the progenitors of type Ia supernovae: binary population synthesis calculations
• Blue straggler stars beyond the Milky Way: a non-segregated population in the Large Magellanic Cloud cluster NGC 2213
• New parameters for star cluster dynamics: the effect of primordial binaries and dark remnants
• Gravitational Waves from Supernova Mass Loss and Natal Kicks in Close Binaries
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
• The properties of long gamma-ray bursts in massive compact binaries
• Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• The long-term evolution of main-sequence binaries in DRAGON simulations
• The population of single and binary white dwarfs of the Galactic bulge
• N-body Simulations with Live Stellar Evolution
• Forming short period sub-stellar companions in 47 Tucanae -- II. Analytic expressions for the orbital evolution of planets in dense environments
• The High Mass X-ray Binaries in star-forming galaxies
• An observational study of rotation and binarity of Galactic O-type runaway stars
• A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)
• Rethinking mass transfer: a unified semianalytical framework for circular and eccentric binaries. II. Orbital evolution due to nonconservative mass transfer
• Merger Conditions of Population III Protostar Binaries
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• Eccentric grazing envelope evolution towards type IIb supernova progenitors
• New Clues to the Evolution of Dwarf Carbon Stars From Their Variability and X-ray Emission
• Progenitor constraints for core-collapse supernovae from Chandra X-ray observations
• Evidence for the Keplerian orbit of a close companion around a giant star
• A Wide Metallicity Range for Gyr-old Stars in the Nuclear Star Cluster
• Introducing a new multi-particle collision method for the evolution of dense stellar systems. Crash-test N-body simulations
• Influence of tidal dissipation on outcomes of binary-single encounters between stars and black holes in stellar clusters
• The Effects of Binary Stars on the Color-Magnitude Diagrams of Young-Age Massive Star Clusters
• Is SN 2006X from a WD + MS system with optically thick wind?
• Tidal Tails of Nearby Open Clusters. II. A Review of Simulated Properties and the Reliability of Observational Catalogues
• The Impact of Astrophysical Priors on Parameter Inference for GW230529
• Weighing the Darkness II: Astrometric Measurement of Partial Orbits with Gaia
• Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
• Rotational synchronisation of B-type binaries in 30 Doradus
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• Binarity at LOw Metallicity (BLOeM): Bayesian inference of natal kicks from inert black hole binaries
• Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars
• The first photometric investigation and spectroscopic analysis of two contact binaries: ASAS J124343+1531.7 and LINEAR 2323566
• The first photometric analysis and period investigation of the K-type W UMa type binary system V0842 Cep
• Characteristics and evolution of Be-type high mass X-ray binaries as potential Ultraluminous X-ray Sources
• Direct N-body simulations of NGC 6397 and its tidal tails
• Exploration of Spin-down Rate of Neutron Star in High Mass X-ray Binaries
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• The effects of Galactic model uncertainties on LISA observations of double neutron stars
• The impact of binary star yields on the spectra of galaxies
• Binary stellar evolution yields in galactic chemical evolution calculations
• New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling
• The role of triple evolution in the formation of LISA double white dwarfs
• Self-Similarities and Power-laws in the Time-resolved Spectra of GRB 190114C, GRB 130427A, GRB 160509A, and GRB 160625B
• Simulating Eclipsing Binary Yields of the Rubin Observatory in the Galactic Field and Star Clusters
• A Strange Star Scenario for the Formation of Eccentric Millisecond Pulsar PSR J1946+3417
• Common envelope evolution and triple dynamics as potential pathways to form the inner white dwarf + brown dwarf binary of the triple star system Gaia 0007-1605
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• Accretion, Ablation and Propeller Evolution in Close Millisecond Pulsar Binary Systems
• Populations of ultraluminous X-ray sources in galaxies: origin and evolution
• LAMOST medium-resolution spectroscopic survey of binarity and exotic star (LAMOST-MRS-B): Observation strategy and target selection
• The Environments around W Serpentis Systems: Independent Limits on System Masses and Extended Envelopes
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• The double helium-white dwarf channel for the formation of AM CVn binaries
• Modeling the progenitors of low-mass post-accretion binaries
• Implications of binary black hole detections on the merger rates of double neutron stars and neutron star-black holes
• A photometric study of two contact binaries: CRTS J025408.1+265957 and CRTS J012111.1+272933
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur
• Are there magnetars in high-mass X-ray binaries?
• Neutron Stars and Black Holes in Star Clusters
• Characteristics of solar-like oscillations of clusters simulated by stellar population synthesis
• The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material
• The Influence of Binary Interactions in Infrared passbands of populations
• Formation of millisecond pulsar-helium star binaries
• Photometric and spectroscopic studies of the long period low mass ratio deep contact binary KN Per
• A Study of Magnetized White Dwarf + Helium Star Binary Evolution to Type Ia Supernovae
• Binary neutron star merger offsets from their host galaxies II. Short-duration gamma-ray bursts
• Orbital eccentricity of the symbiotic star MWC 560
• Made-to-Measure Modelling of Globular Clusters
• The Progeny of Stellar Dynamics and Stellar Evolution within an N-body model of NGC 188
• Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA
• Discovery of pulsating components in eclipsing binary systems through the TESS light curves: The cases of CPD-30 740, HD 97329, V1637 Ori and TYC 683-640-1
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Effect of tides on the orbital evolution of the redback system PSR 1723-2837
• The impact of binary stars on the colors of high-redshift galaxies
• Impact of Asymmetrical Mass Ejection from Proto-White Dwarfs on the Properties of Binary Millisecond Pulsars
• A Unique Low-Mass Ratio Contact Eclipsing Binary System under the Period Cut-Off
• The Origin of Young Stellar Populations in NGC 1783: Accretion of External Stars
• On Isolated Millisecond Pulsars Formed by the Coalescence of Neutron Stars and Massive White Dwarfs
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Wobbling Ancient Binaries - Here Be Planets?
• A Binary Study of Colour-Magnitude Diagrams of 12 Globular Clusters
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Forming short period sub-stellar companions in 47 Tuc: I. Dynamical model and brown dwarf tidal capture rates
• The first photometric investigation of the contact binary OQ Cam
• A photometric and spectroscopic study of eight semi-detached eclipsing binaries
• Hydrodynamical simulations of wind interaction in spider systems : A step toward understanding transitional millisecond pulsars
• Where to find over-massive brown dwarfs: new benchmark systems for binary evolution
• Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
• Multiple stellar populations in MOCCA globular cluster models: Transient spatial over-concentration of pristine red giant stars driven by strong dynamical encounters
• Planetary Systems in a Star Cluster II: intermediate-mass black holes and planetary systems
• Binary Populations of Carbon-Enhanced Metal-Poor Stars
• Dynamical Processes in Globular Clusters
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• An optimal envelope ejection efficiency for merging neutron stars
• The fractions of post-binary-interaction stars and evolved blue straggler stars on the red giant branch of globular clusters
• On the Fast Track: Rapid construction of stellar stream paths
• Photometric analysis and evolutionary stages of the contact binary V2790 Ori
• Interactions among binary black holes in star clusters: Eccentric gravitational wave captures and triple formation
• Ultraluminous X-ray sources in Globular Clusters
• Photometric and spectroscopic observations of the neglected near-contact binary Cl* Melotte 111 AV 1224
• Comparing population synthesis models of compact double white dwarfs to electromagnetic observations
• Co-evolution of Nuclear Star Clusters and Massive Black Holes: Extreme Mass-Ratio Inspirals
• Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
• Calibration of Binary Population Synthesis Models Using White Dwarf Binaries from APOGEE, GALEX and Gaia
• Tidal Synchronization of Binaries in Pleiades
• Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• The Sizes of Globular Clusters as Tracers of Galactic Halo Potentials
• Axisymmetric black hole in a non-commutative gauge theory: classical and quantum gravity effects
• Extended Main Sequences in Star Clusters
• Testing the presence of a dormant black hole inside HR 6819
• Population Synthesis of Gravitational Wave Sources
• Aluminium-26 production in low- and intermediate-mass binary systems
• Binary interactions on the calibrations of star formation rate
• Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729
• First Detailed Analysis of a Relatively Deep, Low Mass-ratio Contact Binary: ATO J108.6991+27.8306
• Quark Novae: An Alternative Channel For the Formation of Isolated Millisecond Pulsars
• Modeling blue stragglers in young clusters
• X-ray binaries with neutron stars at different accretion stages
• Characterisation of the eclipsing post-common-envelope binary TIC 60040774
• Discovery of $\delta$ Sct Components in Eclipsing Binary Systems IQ CMa, AW Men and W Vol
• CXOU J121538.2+361921 in the galaxy NGC 4214: a double neutron star in the making?
• Stripping of a neutron star in a close binary system in a pair with a black hole
• A stringent upper limit on Be star fractions produced by binary interaction
• Past and future of the central double-degenerate core of Henize 2-428
• The cooling time of white dwarfs produced from type Ia supernovae
• Constraints on Population I/II neutron star-black hole binary formation by gravitational wave and radio observations
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Population Synthesis of Massive Close Binary Evolution
• Soft and Supersoft X-ray Sources in Symbiotic Stars
• Progenitors of binary black hole mergers detected by LIGO
• Type Ia Supernovae from First-generation Stars
• The detached, evolved post-mass-exchange binary V643 Orionis
• Formation of millisecond pulsars with wide orbits
• The nature of the X-ray pulsar in M31: an intermediate mass X-ray binary?
• MoBiDICT: new 3D static models of close, synchronized binaries in hydrostatic equilibrium
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Models of Individual Blue Stragglers
• The expected stellar populations in the Kepler and CoRoT fields
• The effects of binary interactions on parameter determinations for early-type galaxies
• Light Axion Emission and the Formation of Merging Binary Black Holes
• Spatial mixing of stellar populations in globular clusters via binary-single star scattering
• Effects of stellar collisions on star cluster evolution and core collapse
• Stellar rotation bifurcation caused by tidal locking in the open cluster NGC 2287?
• Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars
• Pulsars and Millisecond Pulsars III: Tracing Compact Object Dynamics in Globular Clusters with NBODY6++GPU
• Modelling individual globular clusters
• How many VHE gamma-ray binaries with young pulsars can be observed?
• Double white dwarf binary population in MOCCA star clusters -- Comparisons with observations of close and wide binaries
• The impact of stellar rotations and binaries on the shape of upper main sequence near turn off in open cluster NGC\,6067
• FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters
• Mock Observations of Multiple Stellar Populations in Tidal Streams of Palomar 5 for the Chinese Space Station Survey Telescope
• The long-term evolution of Ultra Faint Dwarf Galaxies and observational implications
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
• The explosive life of massive binaries
• Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: II. The long-term evolution of free-floating comets
• Gamma-ray emission from decays of boosted nuclei in protomagnetar jets
• Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
• On the Formation of Eccentric Millisecond Pulsars by Accretion-induced Collapse of Massive White Dwarfs
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• Gravitational waves associated with the r-mode instability from neutron star-white dwarf mergers
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis
• Are most Cataclysmic Variables in Globular Clusters dynamically formed?
• True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
• Interpreting Galaxy Properties with Improved Modelling
• WD + MS systems as the progenitor of SNe Ia
• LISA Galactic Binaries in the Roman Galactic Bulge Time-Domain Survey
• Stellar multiplicity in the Milky Way Galaxy
• Fates of the sub-stellar objects (FOSSO) I. Fates of the known brown dwarfs in main-sequence--BD binaries
• The VLT-FLAMES survey of massive stars. NGC2004#115: A triple system hosting a possible short period B+BH binary
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Population synthesis of neutron star X-ray binaries associated with supernova remnants
• The origin of intergalactic thermonuclear supernovae
• A database of spectral energy distributions of progenitors of core-collapse supernovae
• Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae
• Magnetic dynamos in white dwarfs -III: explaining the occurrence of strong magnetic fields in close double white dwarfs
• Constraining Black Hole Natal Kicks with Astrometric Microlensing
• Using Binaries in Globular Clusters to Catch Sight of Intermediate-Mass Black Holes
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Dynamical double black holes and their host cluster properties
• NGC 2004 #115: a black hole imposter containing three luminous stars
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• 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
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• Inferring binary black holes stellar progenitors with gravitational wave sources
• Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness
• The single degenerate channel for the progenitor of type Ia supernovae
• Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• Six Newly Discovered Eclipsing Binary Systems in the TESS field
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• The Completeness of Accreting Neutron Star Binary Candidates from the Chinese Space Station Telescope
• Gravitational Microlensing Rates in Milky Way Globular Clusters
• Variable Stars in M31 Stellar Clusters from the Panchromatic Hubble Andromeda Treasury
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Are There Pre-Main-Sequence/Black Hole X-ray Binaries?
• Resolving white dwarf binaries within globular clusters with LISA
• Evolving Low- and Intermediate-Mass Binaries: Departures from Classical Theory
• QUEST Eclipsing Binaries and ELLISA: Eclipsing binary search in the QUEST low latitude catalogue and the ELLISA light curve simulator
• Spin-spin coupling in stellar binaries
• Two distributions shedding light on supernova Ia progenitors: delay times and G-dwarf metallicities
• Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network
• The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
• Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots
• Where are Gaia's small black holes?
• The evolution of hierarchical triple star-systems
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• The Role of High-mass Stellar Binaries in the Formation of High-mass Black Holes in Dense Star Clusters
• Constraining Binary Neutron Star Populations using Short Gamma-Ray Burst Observations
• Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• Merging massive black holes: the right place and the right time