Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity

Abstract

We present analytic formulae that approximate the evolution of stars for a wide range of mass and metallicity. Stellar luminosity, radius and core mass are given as a function of age, M and Z, for all phases from the zero-age main-sequence up to, and including, the remnant stages. For the most part we find continuous formulae accurate to within 5% of detailed models. These formulae are useful for purposes such as population synthesis that require very rapid but accurate evaluation of stellar properties, and in particular for use in combination with N-body codes. We describe a mass loss prescription that can be used with these formulae and investigate the resulting stellar remnant distribution.

29 pages, 20 figures, submitted for publication in MNRAS

Cited by in corpus (1269)

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• Relativistic Binary Pulsars with Black-Hole Companions
• Cygnus X-3 and the problem of the missing Wolf-Rayet X-ray binaries
• Merger rate density of binary black holes formed in open clusters
• A-type Stars, the Destroyers of Worlds: The lives and deaths of Jupiters in evolving stellar binaries
• Monte Carlo Simulations of Star Clusters - V. The globular cluster M4
• The Magnetic and Metallic Degenerate G77-50
• Interacting Binaries with Eccentric Orbits. III. Orbital Evolution due to Direct Impact and Self-Accretion
• Internal entrainment and the origin of jet-related broad-band emission in Centaurus A
• The Great Escape II: Exoplanet Ejection from Dying Multiple Star Systems
• Detectability of ultra-compact X-ray binaries as LISA sources
• Six detached white-dwarf close binaries
• The nature of the progenitor of the Type II-P supernova 1999em
• The state of globular clusters at birth II: primordial binaries
• The rapid dispersal of low-mass virialised clusters
• A carbon dwarf wearing a Necklace: first proof of accretion in a post-common-envelope binary central star of a planetary nebula with jets
• GW190412 as a Third-Generation Black Hole Merger from a Super Star Cluster
• Did the infant R136 and NGC 3603 clusters undergo residual gas expulsion?
• Common-Envelope Episodes that lead to Double Neutron Star formation
• Modelling the formation of double white dwarfs
• The Formation of a 70 Msun Black Hole at High Metallicity
• On the kinematics of a runaway Be star population
• Multiple Stellar Evolution: a population synthesis algorithm to model the stellar, binary, and dynamical evolution of multiple-star systems
• Monte Carlo simulations of post-common-envelope white dwarf + main sequence binaries: The effects of including recombination energy
• Evolutionary Population Synthesis for Binary Stellar Populations
• Black hole-neutron star mergers are unlikely multi-messenger sources
• Two white dwarfs in ultrashort binaries with detached, eclipsing, likely substellar companions detected by K2
• IC10~X-1/NGC300~X-1: the very immediate progenitors of BH-BH binaries
• Accreting black hole binaries in globular clusters
• Origin of the S Stars in the Galactic Center
• Galactic Populations of Ultracompact Binaries
• White Dwarf Sequences in Dense Star Clusters
• Complete ejection of OB stars from very young star clusters and the formation of multiple populations
• Tidal Disruptions of Stars by Black Hole Remnants in Dense Star Clusters
• 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
• Close encounters involving free-floating planets in star clusters
• 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3 II: Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures
• Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
• The photometric evolution of star clusters and the preferential loss of low-mass bodies - with an application to globular clusters
• Compact Stellar Binary Assembly in the First Nuclear Star Clusters and r-Process Synthesis in the Early Universe
• White Dwarf Subsystems in Core-Collapsed Globular Clusters
• Impact of a star formation efficiency profile on the evolution of open clusters
• Population synthesis of ultracompact X-ray binaries in the Galactic Bulge
• How Many CVs are Crossing the Period Gap? A Test for the Disruption of Magnetic Braking
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
• 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
• The Effect of Tides on the Population of PN from Interacting Binaries
• Population Synthesis for Symbiotic X-ray Binaries
• Another thread in the tapestry of stellar feedback: X-ray binaries
• MOCCA Survey Database I: Dissolution of tidally filling star clusters harbouring BH subsystems
• A Dynamical N-body Model for the Central Region of $\omega$ Centauri
• No cataclysmic variables missing: higher merger rate brings into agreement observed and predicted space densities
• Tidal Capture of Stars by Intermediate-Mass Black Holes
• Gas depletion in primordial globular clusters due to accretion onto stellar-mass black holes
• Post-common envelope binaries from SDSS - XVI. Long orbital period systems and the energy budget of CE evolution
• A common-envelope wind model for Type Ia supernovae (I): binary evolution and birth rate
• The Age of the Galactic Stellar Halo from Gaia White Dwarfs
• Gaia May Detect Hundreds of Well-characterised Stellar Black Holes
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation III: dissecting black hole dynamics
• An Observational Diagnostic for Ultraluminous X-Ray Sources
• Can Neutron-Star Mergers Explain the r-process Enrichment in Globular Clusters?
• Dynamical Evolution of Multiple-Population Globular Clusters
• $\text{Gaia}$ white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere
• Population synthesis of wide binary millisecond pulsars
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Excitation of oscillation modes by tides in close binaries: constraints on stellar and orbital parameters
• 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
• Binary population synthesis models for core-collapse gamma-ray burst progenitors
• Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah challenge Newtonian gravitation
• Low-mass White Dwarfs with Hydrogen Envelopes as a Missing Link in the Tidal Disruption Menu
• MOCCA-SURVEY Database I: Assessing GW kick retention fractions for BH-BH mergers in globular clusters
• Giant Planets, Tiny Stars: Producing Short-Period Planets around White Dwarfs with the Eccentric Kozai-Lidov Mechanism
• A simple scaling for the minimum instability time-scale of two widely spaced planets
• The Global Mass Functions of 35 Galactic globular clusters: II. Clues on the Initial Mass Function and Black Hole Retention Fraction
• Wind-accreting Symbiotic X-ray Binaries
• Core radius evolution of star clusters
• Population Synthesis of Black Hole Binaries with Normal-Star Companions: I. Detached Systems
• On the minimum mass ratio of W UMa binaries
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Evolution of stellar collision products in open clusters. II. A grid of low-mass collisions
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• The evolution of triples with a Roche-lobe filling outer star
• The White Dwarf Cooling Age of the Open Cluster NGC 2420
• Main-sequence progenitor configurations of the NN Ser candidate circumbinary planetary system are dynamically unstable
• Towards an N-body Model for the Globular Cluster M4
• The stars of the galactic center
• On Rejuvenation in Massive Binary Systems
• A new type of compact stellar population: dark star clusters
• Properties of QSO Metal Line Absorption Systems at High Redshifts: Nature and Evolution of the Absorbers and New Evidence on Escape of Ionizing Radiation from Galaxies
• Influence of a stellar cusp on the dynamics of young stellar discs and the origin of the S-stars in the Galactic Centre
• In Search of the Thermal Eccentricity Distribution
• A perfect starburst cluster made in one go: the NGC 3603 young cluster
• The Past and Future History of Regulus
• The occurrence of Binary Evolution Pulsators in the classical instability strip of RR Lyrae and Cepheid variables
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Light Curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers
• Planetary nebulae after common-envelope phases initiated by low-mass red giants
• Population synthesis of helium white dwarf--red giant star mergers and the formation of lithium-rich giants and carbon stars
• The Size Scale of Star Clusters
• Origin of the early-type R stars: a binary-merger solution to a century-old problem?
• Toward Precision Cosmochronology: A New C/O Phase Diagram for White Dwarfs
• The host galaxies of double compact objects merging in the local Universe
• Exoplanets Beyond the Solar Neighbourhood: Galactic Tidal Perturbations
• Rapidly evolving faint transients from stripped-envelope electron-capture supernovae
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• Alkali metals in white dwarf atmospheres as tracers of ancient planetary crusts
• Discovery of the first wide L dwarf + giant binary system and eight other ultra-cool dwarfs in wide binaries
• A new Monte Carlo method for dynamical evolution of non-spherical stellar systems
• Observed binary populations reflect the Galactic history. Explaining the orbital period-mass ratio relation in wide hot subdwarf binaries
• Predicting Stellar-Mass Black Hole Populations in Globular Clusters
• Masses of the components of the HDE 226868/Cyg X-1 binary system
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• Two Massive White Dwarfs from NGC 2323 and the Initial-Final Mass Relation for Progenitors of 4 to 6.5 M${}_{\odot }$
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• The mass-ratio and eccentricity distributions of barium and S stars, and red giants in open clusters
• The most massive progenitors of neutron stars: CXO J164710.2-455216
• Detection of a $\sim$100,000 M${}_{\odot }$ black hole in M31's most massive globular cluster: A tidally stripped nucleus
• On the formation of compact, massive sub-systems in stellar clusters and its relation with intermediate mass black holes
• The initial mass function of star clusters that form in turbulent molecular clouds
• Indication for an intermediate-mass black hole in the globular cluster NGC 5286 from kinematics
• The Contributions of Interactive Binary Stars to Double Main Sequence Turn-Offs and Dual Red Clump of Intermediate-Age Star Clusters
• Eating Planets for Lunch and Dinner: Signatures of Planet Consumption by Evolving Stars
• The birth rate of SNe Ia from hybrid CONe white dwarfs
• Predicting the hypervelocity star population in Gaia
• Investigating the retention of intermediate-mass black holes in star clusters using N-body simulations
• Consequences of Dynamical Disruption and Mass Segregation for the Binary Frequencies of Star Clusters
• How runaway stars boost galactic outflows
• How to Make a Singleton sdB Star via Accelerated Stellar Evolution
• Combined analysis of neutron star natal kicks using proper motions and parallax measurements for radio pulsars and Be X-ray binaries
• The formation and coalescence sites of the first gravitational wave events
• Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
• Secular dynamics of hierarchical multiple systems composed of nested binaries, with an arbitrary number of bodies and arbitrary hierarchical structure. II. External perturbations: flybys and supernovae
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• WIYN Open Cluster Study XI: WIYN 3.5m Deep Photometry of M35 (NGC 2168)
• Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters
• Biases in the inferred mass-to-light ratio of globular clusters: no need for variations in the stellar mass function
• X1908+075: A Pulsar Orbiting in the Stellar Wind of a Massive Companion
• The helium star donor channel for the progenitors of type Ia supernovae with different metallicities
• White Dwarf Kinematics vs Mass
• Search and analysis of blue straggler stars in open clusters
• Stellar Escape from Globular Clusters. I. Escape Mechanisms and Properties at Ejection
• Modeling the Redshift Evolution of the Normal Galaxy X-ray Luminosity Function
• N-body simulations of globular clusters in tidal fields: Effects of intermediate-mass black holes
• Double Compact Objects as Low-frequency Gravitational Wave Sources
• Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
• The dynamical fate of binary star clusters in the Galactic tidal field
• Spin orbit alignment for KELT-7b and HAT-P-56b via Doppler tomography with TRES
• Double and single recycled pulsars: an evolutionary puzzle?
• Roche-lobe filling factor of mass-transferring red giants - the PIONIER view
• STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
• Helium-Star Mass Loss and its Implications for Black-Hole Formation and Supernova Progenitors
• Constraining the initial mass function of stars in the Galactic Centre
• Dynamics of binary black holes in low-mass young star clusters
• Central kinematics of the globular cluster NGC 2808: Upper limit on the mass of an intermediate-mass black hole
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• Formation of supermassive black hole seeds in nuclear star clusters via gas accretion and runaway collisions
• Buoyant crystals halt the cooling of white dwarf stars
• Survival Rates of Planets in Open Clusters: the Pleiades, Hyades, and Praesepe clusters
• Effective spin distribution of black hole mergers in triples
• On the Spin Period Distribution in Be/X-ray Binaries
• Dark Passengers in Stellar Surveys
• Halo White Dwarfs, Thick Disks and a Sanity Check
• The Detection Rates of Merging Binary Black Holes Originating from Star Clusters and Their Mass Function
• Planetary systems in a star cluster I: the Solar system scenario
• Growth of intermediate mass black holes by tidal disruption events in the first star clusters
• Evolutionary Channels for the Formation of Double Neutron Stars
• Prospects of Finding Detached Black Hole-Star Binaries with TESS
• Transiting exoplanets from the CoRoT space mission XVII. The hot Jupiter CoRoT-17b: a very old planet
• Making massive stars in the Galactic Centre via accretion onto low-mass stars within an accretion disc
• On the Chandra X-ray Sources in the Galactic Center
• Double neutron star mergers from hierarchical triple-star systems
• Two-colour photometry of the binary planetary nebula nuclei UU Sagitte and V477 Lyrae: oversized secondaries in post-common-envelope binaries
• Tidal capture formation of Low Mass X-Ray Binaries from wide binaries in the field
• Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
• Impact of binary interactions on the diffuse supernova neutrino background
• To Ba or not to Ba: Enrichment in s-process elements in binary systems with WD companions of various masses
• A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes
• Helium star evolutionary channel to super-Chandrasekhar mass type Ia supernovae
• A prescription and fast code for the long-term evolution of star clusters - III. Unequal masses and stellar evolution
• Simulations of the Hyades
• MODEST-1: Integrating Stellar Evolution and Stellar Dynamics
• On The Origin Of The Highest Redshift Gamma-Ray Bursts
• The Origins and Evolutionary Status of B Stars Found Far From the Galactic Plane II: Kinematics and Full Sample Analysis
• Evolution models of helium white dwarf--main sequence star merger remnants
• K2-99: a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion
• The fates of Solar system analogues with one additional distant planet
• N-body models of globular clusters: metallicity, half-light radii and mass-to-light ratios
• Population Synthesis of Galactic Be-star Binaries with A Helium-star Companion
• Direct $N$-body simulations of globular clusters - II. Palomar 4
• Hot Jupiters driven by high-eccentricity migration in globular clusters
• SIRIUS Project. III. Star-by-star simulations of star cluster formation using a direct N-body integrator with stellar feedback
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• The Post-Periapse Evolution of Galactic Center Source G1: The second case of a resolved tidal interaction with a supermassive black hole
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• The Pan-Pacific Planet Search VII: The most eccentric planet orbiting a giant star
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• Black hole spins in coalescing binary black holes
• On the Formation of Galactic Black Hole Low-Mass X-ray Binaries
• Mass Evaporation Rate of Globular Clusters in a Strong Tidal Field
• Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• Lithium pollution of a white dwarf records the accretion of an extrasolar planetesimal
• Population synthesis of accreting white dwarfs: II. X-ray and UV emission
• Monte Carlo simulations of star clusters -- III. A million body star cluster
• The theory of globulettes: candidate precursors of brown dwarfs and free floating planets in H II regions
• On the infant weight loss of low- to intermediate-mass star clusters
• The role of stellar collisions for the formation of massive stars
• Speeding past planets? Asteroids radiatively propelled by giant branch Yarkovsky effects
• Populating the Galaxy with pulsars -- II. Galactic dynamics
• 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
• Gamma-ray and X-ray emission from the Galactic Centre: hints on the nuclear star cluster formation history
• On the true shape of the upper end of the stellar initial mass function: The case of R136
• Evolution of Planetary Systems with Time Dependent Stellar Mass Loss
• 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
• White Dwarfs in NGC 6791: Avoiding the Helium Flash
• The growth of massive stars via stellar collisions in ensemble star clusters
• Comparing Compact Object Distributions from Mass- and Presupernova Core Structure-based Prescriptions
• Constraints on single-degenerate Chandrasekhar mass progenitors of Type Iax supernovae
• MASSCLEAN - MASSive CLuster Evolution and ANalysis Package - Description and Tests
• Numerical experiments to help understand cause and effect in massive star evolution
• Trojan Stars in the Galactic Center
• The Origins and Evolutionary Status of B Stars Found Far From the Galactic Plane I: Composition and Spectral Features
• Initial Populations of Black Holes in Star Clusters
• Modest-2: A Summary
• The long-term evolution of star clusters formed with a centrally-peaked star-formation-efficiency profile
• Gaia Reveals Evidence for Merged White Dwarfs
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- I. cataclysmic variables -- present-day population
• Tidal tails of open star clusters as probes to early gas expulsion I: A semi-analytic model
• The M/L ratio of massive young clusters
• Do the majority of stars form as gravitationally unbound?
• Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars
• The Lack of Gamma-Ray Bursts from Population III Binaries
• Spectral analysis of ultra-cool white dwarfs polluted by planetary debris
• Evolution of massive stellar triples and implications for compact object binary formation
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• A new constraint for gamma-ray burst progenitor mass
• A dynamical gravitational wave source in a dense cluster
• Do instabilities in high-multiplicity systems explain the existence of close-in white dwarf planets?
• Post-main-sequence debris from rotation-induced YORP break-up of small bodies II: multiple fissions, internal strengths and binary production
• Clumpy high-z galaxies as a testbed for feedback-regulated galaxy formation
• Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation
• The Galactic Inner Halo: Searching for White Dwarfs and Measuring the Fundamental Galactic Constant, Vo/Ro
• The evolution of the global stellar mass function of star clusters: an analytic description
• On the formation and evolution of the first Be star in a black hole binary MWC 656
• The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function
• DE CVn: A bright, eclipsing red dwarf - white dwarf binary
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• Genesis of magnetic fields in isolated white dwarfs
• How Jupiters save or destroy inner Neptunes around evolved stars
• The state of globular clusters at birth: emergence from the gas-embedded phase
• Dynamical Constraints on the Origin of Multiple Stellar Populations in Globular Clusters
• The Double-Degenerate Nucleus of the Planetary Nebula TS 01. A Close Binary Evolution Showcase
• Roche-lobe overflow systems powered by black holes in young star clusters: the importance of dynamical exchanges
• Astrophysical significance of detection of coalescing binaries with gravitational waves
• The impact of white dwarf natal kicks and stellar flybys on the rates of Type Ia supernovae in triple-star systems
• Return of the TEDI: revisiting the Triple Evolution Dynamical Instability channel in triple stars
• Impact of metallicity on the evolution of young star clusters
• Constraints on the Binary Companion to the SN Ic 1994I Progenitor
• Dynamical Formation of Cataclysmic Variables in Globular Clusters
• The influence of stellar-dynamical ejections and collisions on the relation between the maximum-star and star-cluster-mass
• 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
• Compact Object Modeling in the Globular Cluster 47 Tucanae
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• A statistical view on stable and unstable Roche lobe overflow of a tertiary star onto the inner binary in triple systems
• Pre-explosion companion stars in Type Iax supernovae
• The White Dwarf Binary Pathways Survey -- VIII: a post common envelope binary with a massive white dwarf and an active G-type secondary star
• Eclipsing binaries in extrasolar planet transit surveys: the case of SuperWASP
• The photometric evolution of dissolving star clusters: II. Realistic models. Colours and M/L ratios
• On the Link Between Energy Equipartition and Radial Variation in the Stellar Mass Function of Star Clusters
• The origin of single low-mass WDs: another problem that consequential angular momentum loss in CVs might solve
• First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics
• Understanding the origin of white dwarf atmospheric pollution by dynamical simulations based on detected three-planet systems
• Evolution of the Stellar Mass Function in Multiple-Population Globular Clusters
• Mass modelling globular clusters in the Gaia era: a method comparison using mock data from an $N$-body simulation of M4
• On the Origin of Sub-subgiant Stars. III. Formation Frequencies
• Widespread presence of shallow cusps in the surface-brightness profile of globular clusters
• Early ultraviolet signatures from the interaction of Type Ia supernova ejecta with a stellar companion
• Binary star influence on post-main-sequence multi-planet stability
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• Prospects for detecting asteroseismic binaries in Kepler data
• Some constraints on the lower mass limit for double-degenerate progenitors of Type Ia supernovae
• Black hole - black hole total merger mass and the origin of LIGO/Virgo sources
• An artificial neural network to discover Hypervelocity stars: Candidates in Gaia DR1/TGAS
• Massive black hole assembly in nuclear star clusters
• Prospects for detecting decreasing exoplanet frequency with main sequence age using PLATO
• Acceleration of Cooling of Ice Giants by Condensation in Early Atmospheres
• White Dwarf cooling Sequences, II: luminosity functions
• Companion stars of Type Ia supernovae and single low-mass white dwarfs
• Evolutionary models of short-period soft X-ray transients: comparison with observations
• Radial variation of the stellar mass functions in the globular clusters M15 and M30: clues of a non-standard IMF?
• Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771
• Calibration of neutron star natal kick velocities to isolated pulsar observations
• Massive binary star mergers in galactic nuclei: implications for blue stragglers, binary S-stars and gravitational waves
• Probing Electron-Capture Supernovae: X-Ray Binaries in Starbursts
• The impact of primordial binary on the dynamical evolution of intermediate massive star clusters
• Probing Substellar Companions of AGB Stars through Spirals and Arcs
• Initial-Final Mass Relation for 3 to 4 M${}_{\odot }$ Progenitors of White Dwarfs from the Single Cluster NGC 2099
• Very massive stars in not so massive clusters
• Evidence of a Binary-Induced Spiral from an Incomplete Ring Pattern of CIT 6
• The Binding Energy Parameter for Common Envelope Evolution
• Circumbinary discs for stellar population models
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• FROST: a momentum-conserving CUDA implementation of a hierarchical fourth-order forward symplectic integrator
• Signature of Planetary Mergers on Stellar Spins
• The formation of black hole low-mass X-ray binaries: through case B or case C mass transfer?
• Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all
• Globular cluster formation histories, masses and radii inferred from gravitational waves
• The occurrence of classical Cepheids in binary systems
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• A tale of caution: the tails of NGC 752 are much longer than claimed
• The fate of Cyg X-1: an empirical lower limit on BH-NS merger rate
• Local stellar formation history from the 40 pc white dwarf sample
• V605 Aquilae: a born again star, a nova or both?
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Mass Segregation in NGC 2298: limits on the presence of an Intermediate Mass Black Hole
• On the population III binary black hole mergers beyond the pair-instability mass gap
• Stellar Core-Merger-Induced Collapse: New Formation Pathways for Black Holes, Thorne-$\dot{\mathrm{Z}}$ytkow objects, Magnetars and Superluminous Supernovae
• On measuring the Galactic dark matter halo with hypervelocity stars
• Modeling X-ray binary evolution in normal galaxies: Insights from SINGS
• On the Common Envelope Efficiency
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• Effects of non-Kozai mutual inclinations on two-planet system stability through all phases of stellar evolution
• 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
• The dynamical origin of multiple populations in intermediate-age clusters in the Magellanic Clouds
• Dissecting the Gaia HR diagram within 200 pc
• Do SN 2002cx-like and SN Ia-CSM objects share the same origin?
• Testing the fossil field hypothesis: could strongly magnetised OB stars produce all known magnetars?
• Probing the formation history of the nuclear star cluster at the Galactic Centre with millisecond pulsars
• The Role of "Black Hole Burning" in the Evolution of Dense Star Clusters
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• The connection between merging double compact objects and the Ultraluminous X-ray Sources
• Evolution of star cluster systems in isolated galaxies: first results from direct $N$-body simulations
• Radial Variation in the Stellar Mass Functions of Star Clusters
• A double white dwarf with a paradoxical origin?
• 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
• Population Synthesis of Common Envelope Mergers: I. Giant Stars with Stellar or Substellar Companions
• Binary intermediate-mass black hole mergers in globular clusters
• Neutron star natal kicks and the long-term survival of star clusters
• The gravitational-wave signal generated by a galactic population of double neutron-star binaries
• The MEGaN project I. Missing formation of massive nuclear clusters and tidal disruption events by star clusters - massive black hole interactions
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Matching Globular Cluster Models to Observations
• The coupled effect of tides and stellar winds on the evolution of compact binaries
• Fokker-Planck Models for M15 without a Central Black Hole: The Role of the Mass Function
• Helium-Core White Dwarfs in Globular Clusters
• Binary black hole mergers from young massive clusters in the pair-instability supernova mass gap
• MOCCA-SURVEY Database I: Is NGC 6535 a Dark Star Cluster Harboring an IMBH?
• Stars on the run: escaping from stellar clusters
• Supernova enrichment of planetary systems in low-mass star clusters
• Are white dwarf magnetic fields in close binaries generated during common-envelope evolution?
• Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
• Predictions of a simple parametric model of hierarchical black hole mergers
• Modelling Collision Products of Triple-Star Mergers
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• Exploring compact binary populations with the Einstein Telescope
• The true stellar parameters of the Kepler target list
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• Dynamical modelling of globular clusters: challenges for the robust determination of IMBH candidates
• Exomoons as sources of white dwarf pollution
• The Brightest Point X-Ray Sources in Elliptical Galaxies and the Mass Spectrum of Accreting Black Holes
• The bound mass of Dehnen models with centrally peaked star formation efficiency
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• Demographics of triple systems in dense star clusters
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• The impact of metallicity-dependent mass loss versus dynamical heating on the early evolution of star clusters
• Disrupting Primordial Planet Signatures: The Close Encounter of Two Single-Planet Exosystems in the Galactic Disc
• Population synthesis of neutron stars, strange (quark) stars and black holes
• BIFROST: simulating compact subsystems in star clusters using a hierarchical fourth-order forward symplectic integrator code
• Deep ACS Imaging in the Globular Cluster NGC6397: Dynamical Models
• The Early-type Stars from LAMOST survey: Atmospheric parameters
• Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters
• Blue Large-Amplitude Pulsators: the Possible Surviving Companions of Type Ia Supernovae
• A fast spinning magnetic white dwarf in the double-degenerate, super-Chandrasekhar system NLTT 12758
• Multiwavelength observations of nova SMCN 2016-10a --- one of the brightest novae ever observed
• The IACOB project VIII. Searching for empirical signatures of binarity in fast-rotating O-type stars
• A search for white dwarfs in the Galactic plane: the field and the open cluster population
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• Population synthesis on high-mass X-ray binaries: prospects and constraints from the universal X-ray luminosity function
• MOCCA: Dynamics and evolution of binary stars of multiple stellar populations in tidally filling and underfilling globular star clusters
• Mining for Candidates of Galactic Stellar-mass Black Hole Binaries with LAMOST
• What binary systems are the most likely sources for periodically repeating FRBs?
• The detached-binary channel for the formation of contact binaries
• Magnetic dynamos in white dwarfs -- II. Relating magnetism and pollution
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars
• Roche volume filling and the dissolution of open star clusters
• Dynamical evolution of two-planet systems and its connection with white dwarf atmospheric pollution
• Formation of Black Hole Low-Mass X-ray Binaries
• The impact of massive stars and black holes on the fate of open star clusters and their tidal streams
• A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries
• A population synthesis study on the faint X-ray sources in the Galactic center region
• Formation and Evolution of Ultraluminous X-ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• Revisiting binary stars in population synthesis models
• Compact object detection in self-lensing binary systems with a main-sequence star
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- III. Cataclysmic variables -- Implications of model assumptions
• Detectablity of Black Hole Binaries with Gaia: Dependence on Binary Evolution Models
• Influence of a mass transfer stability criterion on double white dwarf populations
• The role of stellar expansion on the formation of gravitational wave sources
• Discovery of the first resolved triple white dwarf
• The effect of primordial mass segregation on the size scale of globular clusters
• The Blue Stragglers of the Old Open Cluster NGC 188
• The energy transfer and its effects on the secondaries in W Ursae Majoris-type contact binaries
• Black hole-neutron star mergers from triples II: the role of metallicity and spin-orbit misalignment
• Impact of initial mass functions on the dynamical channel of gravitational wave sources
• The chemical composition of TS 01, the most oxygen-deficient planetary nebula. AGB nucleosynthesis in a metal-poor binary star
• Mergers of multi-metallic globular clusters: The role of dynamics
• Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation
• Exploration of the $\ps-\pb$ Relation for Wind-Fed X-Ray Pulsars
• Formation of Very Young Massive Clusters and implications for globular clusters
• Binary black hole mergers from merged stars in the Galactic field
• 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?
• The photometric evolution of dissolving star clusters I: First predictions
• The Curious Case of Palomar 13: The Influence of the Orbital Phase on the Appearance of Galactic Satellites
• On the detection of pre-low-mass X-ray binaries
• Modelling the Observed Stellar Mass Function and its Radial Variation in Galactic Globular Clusters
• Spatial distribution of luminous X-ray binaries in spiral galaxies
• Finding Black Holes with Black Boxes -- Using Machine Learning to Identify Globular Clusters with Black Hole Subsystems
• The viscous evolution of circumstellar discs in young star clusters
• Is there a Size Difference between Red and Blue Globular Clusters?
• The Lifetimes of Star Clusters Born with a Top-heavy IMF
• Revisiting Common Envelope Evolution -- A New Semi-Analytic Model for N-body and Population Synthesis Codes
• Triple evolution: an important channel in the formation of type Ia supernovae
• The birth rate of supernovae from double-degenerate and core-degenerate systems
• Long gamma-ray burst rate at very high redshift
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• Mass-luminosity relation for FGK main sequence stars: metallicity and age contributions
• Imaging an 80 AU Radius Dust Ring Around the F5V Star HD 157587
• Evolution of galaxy habitability
• A Simple Dynamical Model for Omega Cen
• Core radii and common-envelope evolution
• The CO White Dwarf + Intermediate Mass/Massive Star Binary Evolution: Possible Merger Origins for Peculiar Type Ia and II Supernovae
• The Dynamical Evolution of Accreted Star Clusters in the Milky Way
• Formation and Destiny of White Dwarf and Be Star Binaries
• The spin, expansion and contraction of open star clusters
• The Location and Environments of Neutron Star Mergers in an Evolving Universe
• The birth rate of subluminous and overluminous type Ia supernovae
• Applying the metallicity-dependent binary fraction to double white dwarf formation: Implications for LISA
• The black hole retention fraction in star clusters
• LISA sources from young massive and open stellar clusters
• Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant
• The influence of initial mass segregation on the runaway merging of stars
• Hydrodynamic simulations of the central molecular zone with realistic Galactic potential
• Formation and Evolution of Microquasar GRS 1915+105
• $12660$ spotted stars toward the OGLE Galactic bulge fields
• How important is secular evolution for black hole and neutron star mergers in 2+2 and 3+1 quadruple-star systems?
• Observable fractions of core-collapse supernova light curves brightened by binary companions
• Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius--mass relation of embedded clusters
• Metal pollution of the solar white dwarf by solar system small bodies
• New insights in the origin and evolution of the old, metal-rich open cluster NGC 6791
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• H2 chemistry in galaxy simulations: an improved supernova feedback model
• Linking the formation and fate of exo-Kuiper belts within solar system analogues
• The entry geometry and velocity of planetary debris into the Roche sphere of a white dwarf
• Expected masses of merging compact object binaries observed in gravitational waves
• A prescription and fast code for the long-term evolution of star clusters - II. Unbalanced and core evolution
• MOCCA code for star cluster simulations - VI. Bimodal spatial distribution of blue stragglers
• The "DODO" survey I: limits on ultra-cool substellar and planetary-mass companions to van Maanen's star (vMa 2)
• Formation constraints indicate a black-hole accretor in 47 Tuc X9
• On the absence of symbiotic stars in globular clusters
• The critical binary star separation for a planetary system origin of white dwarf pollution
• The s-process in stellar population synthesis: a new approach to understanding AGB stars
• Oxygen-neon rich merger during common envelope evolution
• Evolutionary Constraints on the Planet-Hosting Subgiant Epsilon Reticulum from its White Dwarf Companion
• A new candidate Wolf-Rayet X-ray binary in NGC 253
• Hyades dynamics from N-body simulations: Accuracy of astrometric radial velocities from Hipparcos
• Binary interactions as a possible scenario for the formation of multiple stellar populations in globular clusters
• Population synthesis of accreting white dwarfs: Rates and evolutionary pathways of H and He novae
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• Probability Distribution of Terrestrial Planets in Habitable Zones around Host Stars
• Companion Stars of Type Ia supernovae with different metallicities
• Transiting exoplanets from the CoRoT space mission XXVII. CoRoT-28b, a planet orbiting an evolved star, and CoRoT-29b, a planet showing an asymmetric transit
• Contribution of primordial binary evolution to the two blue-straggler sequences in globular cluster M30
• 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
• Star Clusters Under Stress: Why Small Systems Cannot Dynamically Relax
• Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters
• Modified gravity in the interior of population II stars
• Forming Hot Subluminous Stars from Hierarchical Triples -- I. The Role of an Outer Tertiary on Formation Channels
• Runaway and Hypervelocity Stars from Compact Object Encounters in Globular Clusters
• Unseen companions of V Hya inferred from periodic ejections
• Evolution of Helium Star - White Dwarf Binaries Leading up to Thermonuclear Supernovae
• Constraining planet formation around 6$M_{\odot }$-8$M_{\odot }$ stars
• A Population of Neutron Star Ultraluminous X-ray Sources with A Helium Star Companion
• Potential Importance of Binary Evolution in UV-Optical Spectral Fitting of Early-Type Galaxies
• Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
• Relaxation near supermassive black holes driven by nuclear spiral arms: anisotropic hypervelocity stars, S-stars and tidal disruption events
• Merging of a CO WD and a He-rich white dwarf to produce a type Ia supernovae
• Forward Modelling the O3(a+b) GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions
• Dynamical formation of Black Hole Low-Mass X-Ray Binaries in the field - an alternative to common envelope
• Testing lowered isothermal models with direct N-body simulations of globular clusters - II: Multimass models
• Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
• The impact of metallicity on nova populations
• Close stellar encounters at the Galactic Centre I: The effect on the observed stellar populations
• MOCCA-SURVEY Database II -- Properties of Intermediate Mass Black Holes escaping from star clusters
• Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way
• TIC 308396022: a $\delta$ Scuti--$\gamma$ Doradus hybrid with large-amplitude radial fundamental mode and regular g-mode period spacing
• Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*
• Integrated Spectral Energy Distributions and Absorption Feature Indices of Single Stellar Populations
• The most metal-rich asymptotic giant branch stars
• Wind-powered ultraluminous X-ray sources
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: possible detection of an ejected common envelope
• Black Holes In Young Stellar Clusters
• The star cluster survivability after gas expulsion is independent of the impact of the Galactic tidal field
• The contribution of dissolving star clusters to the population of ultra-faint objects in the outer halo of the Milky Way
• Two paths of cluster evolution: global expansion versus core collapse
• Stellar-mass black holes in the Hyades star cluster?
• Mergers of neutron stars and black holes with cores of giant stars: a population synthesis study
• 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
• Collective Properties of X-ray Binary Populations of Galaxies. I. Luminosity and Orbital Period Distributions of High-Mass X-ray Binaries
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
• Dynamically Formed Black Hole Binaries: In-Cluster Versus Ejected Mergers
• The smallest planetary drivers of white dwarf pollution
• A Fallback Disk Accretion-Involved Formation Channel to PSR J1903+0327
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- II. Cataclysmic variables -- progenitors and population at birth
• A Triple Star Origin For T Pyx and Other Short-Period Recurrent Novae
• 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
• The Destruction of an Oort Cloud in a rich stellar cluster
• Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes
• A numerical study of stellar discs in galactic nuclei
• Star Cluster Evolution in Dark Matter Dominated Galaxies
• Efficiency of black hole formation via collisions in stellar systems: An analysis of data from simulations and observations
• Gravitational-wave radiation from double compact objects with eLISA in the Galaxy
• Tidal disruption events onto stellar black holes in triples
• A strange star scenario for the formation of isolated millisecond pulsars
• Rates and delay times of Type Ia supernovae in the helium-enriched main-sequence donor scenario
• The Spectral Evolution of Convective Mixing White Dwarfs, the non-DA Gap, and White Dwarf Cosmochronology
• MOCCA code for star cluster simulations - V. Initial globular cluster conditions influence on blue stragglers
• Lower-mass-gap Black Holes in Dense Star Clusters
• Simplified galaxy formation with mesh-less hydrodynamics
• A New Hybrid Technique for Modeling Dense Star Clusters
• Millisecond pulsars and the gamma-ray excess in Andromeda
• A Monte Carlo study of early gas expulsion and evolution of star clusters: new simulations with the MOCCA code in the AMUSE framework
• Accretion mode of the Ultra-Luminous X-ray source M82 X-2
• Post-merger evolution of double helium white dwarfs and distribution of helium-rich hot subdwarfs
• How does a low-mass cut-off in the stellar IMF affect the evolution of young star clusters?
• Rapidly rotating neutron star progenitors
• The formation of subdwarf A-type stars
• TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars
• Mass segregation and dynamics of primordial binaries in star clusters with a radially anisotropic velocity distribution
• Star Cluster Formation from Turbulent Clumps. III. Across the mass spectrum
• The envelope mass of red giant donors in Type Ia supernova progenitors
• A wind-blown bubble in the Central Molecular Zone cloud G0.253+0.016
• Wandering off the centre: a characterization of the random motion of intermediate-mass black holes in star clusters
• Star formation history, double degenerates and type Ia supernovae in the thin disc
• The influence of star formation history on the gravitational wave signal from close double degenerates in the thin disc
• Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations
• The Effect of Stellar Metallicity on the Sizes of Star Clusters
• Star Cluster Formation from Turbulent Clumps. I. The Fast Formation Limit
• Eclipsing binary statistics - theory and observation
• Targeted modeling of GW150914's binary black hole source with dart_board
• Modeling Hot Gas Flow in the Low-Luminosity Active Galactic Nucleus of NGC3115
• Three new barium dwarfs with WD companions: BD+68 1027, RE J0702+129 and BD+80 670
• Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars
• Simulating Star Clusters with the AMUSE Software Framework: I. Dependence of Cluster Lifetimes on Model Assumptions and Cluster Dissolution Modes
• GalevNB: a conversion from N-BODY simulations to observations
• A class of spherical, truncated, anisotropic models for application to globular clusters
• NGTS-12b: A sub-Saturn mass transiting exoplanet in a 7.53 day orbit
• Mergers prompted by dynamics in compact, multiple-star systems: a stellar-reduction case for the massive triple TIC 470710327
• The galactic rate of second and third generation disc and planet formation
• On the Formation of Runaway Stars BN and x in the Orion Nebula Cluster
• The mass distribution of stars stripped in binaries: The effect of metallicity
• Hunting intermediate-mass black holes with LISA binary radial velocity measurements
• Formation of black hole X-ray binaries with non-degenerate donors in globular clusters
• Hot subdwarf B stars with neutron star components II: Binary population synthesis
• Repeated mergers of black hole binaries: implications for GW190521
• On the dynamical evolution of Cepheids in star clusters
• The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
• Binary population synthesis study on supersoft X-ray phase of single degenerate type Ia supernova progenitors
• Galactic orbital motions of star clusters: static versus semicosmological time-dependent Galactic potentials
• Magnesium-rich Ejecta in the SNR G284.3$-$1.8 Around the High-Mass Gamma-Ray Binary 1FGL J1018.6$-$5856
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?
• Unraveling the Formation History of the Black Hole X-ray Binary LMC X-3 from ZAMS to Present
• The effects of stellar population synthesis on the distributions of the asteroseismic observables ν_max and Δν of red-clump stars
• Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
• The unstable fate of the planet orbiting the A-star in the HD 131399 triple stellar system
• The Formation of Binary Star Clusters in the Milky Way and Large Magellanic Cloud
• Circumstellar properties of Type Ia supernovae from the helium star donor channel
• Globular clusters as probes of dark matter cusp-core transformations
• Low-mass X-ray Binaries with Strange Quark Stars
• Gaia BH1 and BH2 -- evolutionary models with overshooting of the black hole progenitors within the present-day binary separation
• Finding White Dwarfs with Transit Searches
• Constraining mass transfer and common-envelope physics with post-supernova companion monitoring
• Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
• Variation in the Stellar Mass Function Along Stellar Streams
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• On the Rarity of X-Ray Binaries with Naked Helium Donors
• Predictions for Triple Stars with and without a Pulsar in Star Clusters
• The post-main-sequence fate of the HR 8799 planetary system
• The grain size survival threshold in one-planet post-main-sequence exoplanetary systems
• Disentangling the parameter space: The role of planet multiplicity in triggering dynamical instabilities on planetary systems around white dwarfs
• Spatial and Binary Parameter Distributions of Black Hole Binaries in the Milky Way Detectable with Gaia
• The impact of binaries on the evolution of star clusters from turbulent molecular clouds
• The Mass and Age Distribution of Halo White Dwarfs in the Canada-France Imaging Survey
• HD 76920b pinned down: a detailed analysis of the most eccentric planetary system around an evolved star
• Red giant depletion in globular cluster cores
• On the origin of the split main sequences of the young massive cluster NGC 1856
• New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
• The effect of metallicity on the delay-time distribution of type Ia supernova
• Constraining the star formation rate with the extragalactic background light
• Probing the Survival of Planetary Systems in Globular Clusters with Tidal Disruption Events
• On the Tidal Capture of White Dwarfs by Intermediate-mass Black Holes in Dense Stellar Environments
• The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles
• Stellar winds near massive black holes: The case of the S-stars
• Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• MOCCA Survey Database: Extra Galactic Globular Clusters. I. Method and first results
• MOCCA: Global properties of tidally filling and underfilling globular star clusters with multiple stellar populations
• Electromagnetic transients and gravitational waves from white dwarf disruptions by stellar black holes in triple systems
• Energy equipartition in multiple-population globular clusters
• The rate of iPTF 14gqr like ultra-stripped supernovae and binary evolution leading to double neutron star formation
• Cataclysmic Variables in Triples: Formation Models and New Discoveries
• The Early Evolution of Star Clusters in Compressive and Extensive Tidal Fields
• On asymmetric dark matter constraints from the asteroseismology of a subgiant star
• Binary Star Population with Common Proper Motion in Gaia DR2
• Primordial mass segregation of star clusters with primordial binaries
• The Population of Helium-Merger Progenitors: Observational Predictions
• Gravitational lensing as a probe of compact object population in the Galaxy
• IP Eri: A surprising long-period binary system hosting a He white dwarf
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• High resolution ALMA and HST imaging of $\kappa$CrB: a broad debris disc around a post-main sequence star with low-mass companions
• Spin evolution of neutron stars in wind-fed high mass X-ray binaries
• Chemical abundances of primary stars in the Sirius-like binary systems
• GABE: Galaxy Assembly with Binary Evolution
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
• Correlation Between Mass Segregation and Structural Concentration in Relaxed Stellar Clusters
• Monte Carlo simulations of multiple populations in globular clusters: constraints on the initial size of the second generation from binary stars
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• Pre-mainsequence stellar evolution in N-body models
• Simulating stellar winds in AMUSE
• Binary Natal Kicks in the Galactic Center: X-ray Binaries, Hypervelocity Stars, and Gravitational Waves
• Mass-stream trajectories with non-synchronously rotating donors
• The possible existence of Pop III NS-BH binary and its detectability
• Mergers all the way down: stellar collisions and kinematics of a dense hierarchically forming massive star cluster in a dwarf starburst
• Scalable stellar evolution forecasting: Deep learning emulation vs. hierarchical nearest neighbor interpolation
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Analytic approximations for massive close post-mass transfer binary systems
• The Effect of Stellar Helium Abundance on Dynamics of Multiple Populations in Globular Clusters
• The Yarkovsky effect in REBOUNDx
• Can star cluster environment affect dust input from massive AGB stars?
• The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes
• Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters
• WD + He star systems as the progenitors of Type Ia supernovae and their surviving companion stars
• High-Mass X-Ray Binaries with Be Donors as Ultraluminous X-Ray Sources
• The Starlab Environment for Dense Stellar Systems
• Evolution models of helium white dwarf--main-sequence star merger remnants: the mass distribution of single low-mass white dwarfs
• Common Envelope Mechanisms: Constraints from the X-ray Luminosity Function of High Mass X-ray Binaries
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• The mass, luminosity and mass-loss rate of the donor of the V1487 Aql/GRS 1915+105 binary system
• McScatter: a Simple Three-Body Scattering Package with Stellar Evolution
• Wide binary pulsars from electron-capture supernovae
• Can eccentric binary millisecond pulsars form by accretion induced collapse of white dwarfs?
• Multi-scale and multi-domain computational astrophysics
• An Empirical Fit for Viscoelastic Simulations of Tertiary Tides
• Long gamma ray burst rate in the binary merger progenitor model
• Making hot Jupiters in stellar clusters: the importance of binary exchange
• Mechanisms for high spin in black-hole neutron-star binaries and kilonova emission: inheritance and accretion
• On the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth
• Testing the mass-radius relation of white dwarfs in common proper motion pairs I.Hydrogen-dominated atmospheres
• The Ages of M31 Star Clusters: Spectral Energy Distribution Versus Color-Magnitude Diagram
• Binary Population Synthesis: Methods, Normalization, and Surprises
• 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
• A binary origin for the first isolated stellar-mass black hole detected with astrometric microlensing
• Millisecond Pulsars in Dense Star Clusters: Evolution, Scaling Relations, and the Galactic-Center Gamma-ray Excess
• A closer look at non-interacting He stars as a channel for producing the old population of Type Ia supernovae
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• Can the Subsonic Accretion Model Explain the Spin Period Distribution of Wind-fed X-ray Pulsars?
• The mass distribution of stellar mergers: A new scenario for several FS CMa stars
• Unveiling the Binary Nature of NGC 2323
• Yunnan-III models for Evolutionary population synthesis
• Statistics of Magrathea exoplanets beyond the Main Sequence. Simulating the long-term evolution of circumbinary giant planets with TRES
• Influence of planets on debris disks in star clusters I: the 50 AU Jupiter
• GPU-Accelerated Periodic Source Identification in Large-Scale Surveys: Measuring $P$ and $\dot{P}$
• The phase curve of the ultra-hot Jupiter WASP-167b as seen by TESS
• Formation rate of LB-1-like systems through dynamical interactions
• Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product
• Binary imposters: Mergers in massive hierarchical triple stars
• A Be Star + He Star Binary as an Indicator of a Binary Mass Transfer Phase
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Potential for life to exist and be detected on Earth-like planets orbiting white dwarfs
• Population Study of Astrophysical False Positive Detections in the Southern PLATO field
• Blue straggler stars beyond the Milky Way: a non-segregated population in the Large Magellanic Cloud cluster NGC 2213
• On the Formation of SS433
• Phase-space mixing of multiple stellar populations in globular clusters
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Lost in space: companions' fatal dance around massive dying stars
• Flare Activity and Magnetic Feature Analysis of the Flare Stars II: Sub-Giant Branch
• The Initial Properties of Young Star Clusters in M83
• Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A
• The effects of UV photometry and binary interactions on photometric redshift and galaxy morphology
• TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet
• Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors
• X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
• Probing the formation of planetesimals in the Galactic Centre using Sgr A* flares
• Investigating the UV-excess in star clusters with $N$-body simulations: predictions for future CSST observations
• Population synthesis of hot subdwarf B stars with COMPAS: on the observed Galactic population
• High-resolution resonant portraits of a single-planet white dwarf system
• WD mass and orbital period relation of sdB + He WD binaries
• MOCCA: Effects of pristine gas accretion and cluster migration on globular cluster evolution, global parameters, and multiple stellar populations
• Precision Astrometry of the Exoplanet Host Candidate GD 66
• A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
• Compact objects formation, retention, and growth through accretion onto gas-embedded white-dwarfs/neutron-stars in gas-enriched globular-clusters
• Gravitational Dynamics of Large Stellar Systems
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• Massive stellar triples on the edge: A numerical study of the evolution and final outcomes of destabilized massive triples
• Mathematical encoding within multi-resonant planetary systems as SETI beacons
• Dynamics of passing-stars-perturbed binary star systems
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• 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?
• Heavy element contributions of rotating massive stars to Interstellar Medium
• Introducing a new multi-particle collision method for the evolution of dense stellar systems. Crash-test N-body simulations
• N-body Simulations with Live Stellar Evolution
• Tidal Tails of Nearby Open Clusters. II. A Review of Simulated Properties and the Reliability of Observational Catalogues
• Forming short period sub-stellar companions in 47 Tucanae -- II. Analytic expressions for the orbital evolution of planets in dense environments
• The Impact of Astrophysical Priors on Parameter Inference for GW230529
• A white dwarf bound to the transiting planetary system WASP-98
• New parameters for star cluster dynamics: the effect of primordial binaries and dark remnants
• The long-term evolution of main-sequence binaries in DRAGON simulations
• The symbiotic binary St 2-22: Orbital and stellar parameters and jet evolution following its 2019 outburst
• Planetary magnetosphere evolution around post-main-sequence stars
• Blue Stragglers in Globular Clusters: Observations, Statistics and Physics
• Bulge Fossil Fragments as a new population of factories of gravitational wave sources in the Galaxy
• The role of triple evolution in the formation of LISA double white dwarfs
• The Effect of Pre-Main Sequence Stars on Star Cluster Dynamics
• Direct N-body simulations of NGC 6397 and its tidal tails
• The Influence of Binary Interactions in Infrared passbands of populations
• Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• Characteristics of solar-like oscillations of clusters simulated by stellar population synthesis
• Exploration of Spin-down Rate of Neutron Star in High Mass X-ray Binaries
• Local merger rates of double neutron stars
• A Strange Star Scenario for the Formation of Eccentric Millisecond Pulsar PSR J1946+3417
• Are there magnetars in high-mass X-ray binaries?
• Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
• Accretion, Ablation and Propeller Evolution in Close Millisecond Pulsar Binary Systems
• 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
• Tracking Cluster Debris (TraCD)- I. Dissolution of clusters and searching the solar cradle
• Characteristics and evolution of Be-type high mass X-ray binaries as potential Ultraluminous X-ray Sources
• Binary stellar evolution yields in galactic chemical evolution calculations
• The double helium-white dwarf channel for the formation of AM CVn binaries
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• On the Fast Track: Rapid construction of stellar stream paths
• Collective Properties of X-ray Binary Populations of Galaxies II. Pre-Low-mass X-ray Binary Properties, Formation Rates, and Constraints
• Orbital Separation Amplification in Fragile Binaries with Evolved Components
• On Isolated Millisecond Pulsars Formed by the Coalescence of Neutron Stars and Massive White Dwarfs
• The impact of binary stars on the colors of high-redshift galaxies
• Intermediate-mass black holes in globular clusters: observations and simulations
• Average Inhomogeneities in Milky Way SNII and The PAMELA Anomaly
• An optimal envelope ejection efficiency for merging neutron stars
• Constellations of co-orbital planets: horseshoe dynamics, long-term stability, transit timing variations, and potential as SETI beacons
• Tracing the Evolution of SMBHs and Stellar Objects in Galaxy Mergers: An Multi-mass Direct N-body Model
• Nature of donors in ultra-luminous X-ray binaries powered by neutron stars
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Unveiling Bifurcated Blue Straggler Sequences in NGC 2173: Insights from Binary Evolution
• Dark Star Clusters or Ultra-Faint Dwarf galaxies? Revisiting UMa3/U1
• The Progeny of Stellar Dynamics and Stellar Evolution within an N-body model of NGC 188
• Multiple stellar populations in MOCCA globular cluster models: Transient spatial over-concentration of pristine red giant stars driven by strong dynamical encounters
• Interactions among binary black holes in star clusters: Eccentric gravitational wave captures and triple formation
• Ultraluminous X-ray sources in Globular Clusters
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Dynamical Processes in Globular Clusters
• Emulators for stellar profiles in binary population modeling
• Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA
• Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• The Origin of Young Stellar Populations in NGC 1783: Accretion of External Stars
• The fractions of post-binary-interaction stars and evolved blue straggler stars on the red giant branch of globular clusters
• Made-to-Measure Modelling of Globular Clusters
• Planetary Systems in a Star Cluster II: intermediate-mass black holes and planetary systems
• Forming short period sub-stellar companions in 47 Tuc: I. Dynamical model and brown dwarf tidal capture rates
• Population Synthesis of Gravitational Wave Sources
• Effect of dynamical interactions on integrated properties of globular clusters
• Calibration of Binary Population Synthesis Models Using White Dwarf Binaries from APOGEE, GALEX and Gaia
• Spatial mixing of stellar populations in globular clusters via binary-single star scattering
• 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
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• The effects of binary interactions on parameter determinations for early-type galaxies
• Binary-single interactions with different mass ratios
• Tidal Synchronization of Binaries in Pleiades
• Observational properties of visual binaries as modelled using a synthetic catalogue, I: For visual apparent magnitudes $m_v<15$
• The nature of the X-ray pulsar in M31: an intermediate mass X-ray binary?
• Helium emission from Balmer-dominated shocks in Type Ia supernova remnants provides constraints to their progenitor systems
• Influence of irradiation-driven winds on the evolution of intermediate-mass black hole X-ray binaries
• Habitable Zones of Host Stars During the Post-MS Phase
• Testing the presence of a dormant black hole inside HR 6819
• Binary interactions on the calibrations of star formation rate
• Origin of High Dark Remnant Fractions in Milky Way Globular Clusters: The Crucial Role of Initial Black Hole Retention
• The cooling time of white dwarfs produced from type Ia supernovae
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Aluminium-26 production in low- and intermediate-mass binary systems
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• The Sizes of Globular Clusters as Tracers of Galactic Halo Potentials
• Characterisation of the eclipsing post-common-envelope binary TIC 60040774
• Past and future of the central double-degenerate core of Henize 2-428
• A Recent Supermassive Black Hole Binary in the Galactic Center Unveiled by the Hypervelocity Stars
• X-ray binaries with neutron stars at different accretion stages
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Stripping of a neutron star in a close binary system in a pair with a black hole
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Constraints Between Equations of State and Mass-Radius Relationships in General Clusters of Stellar Systems
• WD + MS systems as the progenitor of SNe Ia
• How many VHE gamma-ray binaries with young pulsars can be observed?
• Constraining the progenitor evolution of GW 150914
• New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences
• Exoplanet Nodal Precession Induced by Rapidly Rotating Stars: Impacts on Transit Probabilities and Biases
• Evolutionary models of the optical component of the LMC X-1/Star 32 binary system
• The X-ray binaries in M83: will any of them form gravitational wave sources for LIGO/VIRGO/KAGRA?
• Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: II. The long-term evolution of free-floating comets
• Mock Observations of Multiple Stellar Populations in Tidal Streams of Palomar 5 for the Chinese Space Station Survey Telescope
• A new third planet and the dynamical architecture of the HD33142 planetary system
• Constraints on Weak Supernova Kicks from Observed Pulsar Velocities
• Double white dwarf binary population in MOCCA star clusters -- Comparisons with observations of close and wide binaries
• Fates of the sub-stellar objects (FOSSO) I. Fates of the known brown dwarfs in main-sequence--BD binaries
• True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
• The long-term evolution of Ultra Faint Dwarf Galaxies and observational implications
• FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters
• Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
• Modelling individual globular clusters
• TOI-1259Ab: A Warm Jupiter Orbiting a K-dwarf White-Dwarf Binary is on a Well-aligned Orbit
• Towards systematic searches for LISA white dwarf binaries with multiband photometry
• On the Formation of Eccentric Millisecond Pulsars by Accretion-induced Collapse of Massive White Dwarfs
• Dynamical double black holes and their host cluster properties
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• Gravitational Microlensing Rates in Milky Way Globular Clusters
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae
• Gravitational background from dynamical binaries and detectability with 2G detectors
• The mass-to-light ratio of rich star clusters
• Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations
• Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots
• A database of spectral energy distributions of progenitors of core-collapse supernovae
• The mmax-Mecl relation in the LEGUS clusters
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• One's loss is (not) another's gain: Isotropic re-emission destabilizes mass transfer from radiative donor stars
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• White dwarfs in the building blocks of the Galactic spheroid
• Resolving white dwarf binaries within globular clusters with LISA
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Merger rates of intermediate-mass black hole binaries in nuclear star clusters
• A new method to retrieve the star formation history from white dwarf luminosity functions -- an application to the Gaia catalogue of nearby stars
• Primordial helium-3 redux: The helium isotope ratio of the Orion nebula
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• The single degenerate channel for the progenitor of type Ia supernovae
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• The Completeness of Accreting Neutron Star Binary Candidates from the Chinese Space Station Telescope
• Revisiting the Evolutionary Status of Massive Stars at the central parsec of the Milky Way
• Star Cluster Simulations Including Stellar Evolution