X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
arXiv:2501.12507 · doi:10.1051/0004-6361/202553829
Abstract
Tidally induced spin-up of stripped helium stars in short-period (<\,1\,d) binaries with black holes has been presented as one of the possible mechanisms to reproduce the high-spin tail of the black hole spin distribution derived from gravitational wave (GW) merger observations. At such short periods, a fraction of the strong stellar wind from the stripped helium stars may be accreted by the black holes, and its gravitational potential energy may be released as observable radiation in the X-ray regime. We estimate the X-ray luminosity and its observability from black holes in orbit with stripped helium stars, which evolve into binary black hole or black hole+neutron star binaries that merge within Hubble time. We post-process recent advancements for estimating X-ray luminosities (via wind accretion onto stellar mass black holes) into two rapid population synthesis codes, BSE and StarTrack. We derive lower limits on the X-ray luminosity distribution from populations of stripped helium+black hole binaries at four metallicities (0.01, 0.1, 0.5, 1 ) and two mass transfer stability criteria. We find that a large fraction (0.1-0.5) of stripped-helium stars that get spun up by tides also transfer enough wind matter onto the black hole to produce X-ray luminosities above \,erg\,s, up to \,erg\,s. Such binaries should be observable as X-ray bright systems at 0.1\,, 0.5\, and , representative of Sextans A, the Large Magellanic Cloud (LMC) and the Solar neighbourhood, respectively. The formation efficiency of these systems increases with decreasing metallicity. However, accounting for the local star formation rates, our population synthesis predicts 2 and 1 such observable binaries in the Milky Way and LMC, respectively, that will produce a binary compact object merger within a Hubble time. (Abridged)
accepted in A&A
References in corpus (112)
- On the variation of the Initial Mass Function
- Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
- Binary interaction dominates the evolution of massive stars
- Evolution of binary stars and the effect of tides on binary populations
- Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
- Mass-loss predictions for O and B stars as a function of metallicity
- Advection-Dominated Accretion: Underfed Black Holes and Neutron Stars
- A statistical study of 233 pulsar proper motions
- Common Envelope Evolution: Where we stand and how we can move forward
- Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
- Dynamo action by differential rotation in a stably stratified stellar interior
- Compact Object Modeling with the StarTrack Population Synthesis Code
- Ultraluminous X-Ray Sources in External Galaxies
- Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
- Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
- Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
- The Star Formation History of the Large Magellanic Cloud
- The Effect of Pair-Instability Mass Loss on Black Hole Mergers
- Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE
- The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere
- The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes
- The Mass of the Black Hole in Cygnus X-1
- On the formation and evolution of black-hole binaries
- Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
- Most Black Holes are Born Very Slowly Rotating
- One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
- Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
- Cygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds
- Merging black hole binaries with the SEVN code
- Missing Black Holes Unveil The Supernova Explosion Mechanism
- The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO
- The spin of the second-born black hole in coalescing binary black holes
- The Galactic WC stars: Stellar parameters from spectral analyses indicate a new evolutionary sequence
- Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
- The Radiative Efficiency of Hot Accretion Flows
- Stability of mass transfer from massive giants: double black-hole binary formation and ultra-luminous X-ray sources
- The role of mass transfer and common envelope evolution in the formation of merging binary black holes
- The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Gamma-dependence of Wolf-Rayet type mass loss
- A New Dynamical Model for the Black Hole Binary LMC X-1
- Different to the core: the pre-supernova structures of massive single and binary-stripped stars
- The impact of mass-transfer physics on the observable properties of field binary black hole populations
- Ultraluminous X-ray sources
- The expansion of stripped-envelope stars: consequences for supernovae and gravitational-wave progenitors
- The redshift evolution of the binary black hole merger rate: a weighty matter
- The Origin of Black Hole Spin in Galactic Low-Mass X-ray Binaries
- BSE versus StarTrack: implementations of new wind, remnant-formation, and natal-kick schemes in NBODY7 and their astrophysical consequences
- Constraints on Binary Black Hole Populations from LIGO-Virgo Detections
- GW150914: Spin based constraints on the merger time of the progenitor system
- Distribution of Effective Spins and Masses of Binary Black Holes from the LIGO and Virgo O1-O3a Observing Runs
- Gamma-Ray Bursts from tidally spun-up Wolf-Rayet stars?
- Stellar-mass black holes in young massive and open stellar clusters IV: updated stellar-evolutionary and black hole spin models and comparisons with the LIGO-Virgo O1/O2 merger-event data
- Cyg X-3: a low-mass black hole or a neutron star
- The most ordinary formation of the most unusual double black hole merger
- Be X-ray binaries in the SMC as indicators of mass transfer efficiency
- Binary black hole mergers: formation and populations
- Massive donors in interacting binaries: effect of metallicity
- Detailed models of interacting short-period massive binary stars
- Synthetic catalog of black holes in the Milky Way
- The impact of common envelope development criteria on the formation of LIGO/Virgo sources
- First Stellar Abundances in the Dwarf Irregular Galaxy Sextans A
- The Star Formation Rate of the Milky Way as seen by Herschel
- The spins of compact objects born from helium stars in binary systems
- The implications of high BH spins on the origin of BH-BH mergers
- Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
- Photometric metallicity map of the Large Magellanic Cloud
- The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
- Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
- Red Supergiants as Cosmic Abundance Probes: The Magellanic Clouds
- The Effect of Supernova Convection On Neutron Star and Black Hole Masses
- A two-stage formalism for common-envelope phases of massive stars
- A Population of Ultraluminous X-ray Sources with An Accreting Neutron Star
- Population Synthesis of Black Hole Binaries with Normal-Star Companions: I. Detached Systems
- Bounds on Expected Black Hole Spins in Inspiraling Binaries
- The temperature dependency of Wolf-Rayet-type mass loss: An exploratory study for winds launched by the hot iron bump
- Population Synthesis of Black Hole X-Ray Binaries
- Ultra-compact X-ray binaries with He star companions
- The VMC survey -- XLIV: Mapping metallicity trends in the Large Magellanic Cloud using near-infrared passbands
- Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes
- Systematically Revisiting All NuSTAR Spins of Black Holes in X-Ray Binaries
- Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants
- Tidal Spin-up of Black Hole Progenitor Stars
- Explaining the differences in massive star models from various simulations
- Black-hole mergers in disklike environments could explain the observed - correlation
- A dearth of young and bright massive stars in the Small Magellanic Cloud
- Gravitational waves from in-spirals of compact objects in binary common-envelope evolution
- X-ray emission from BH+O star binaries expected to descend from the observed galactic WR+O binaries
- Evidence from high mass X-ray binaries that Galactic WR components of WR+O binaries end their life with a supernova explosion
- Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
- Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
- Prospects of gravitational-waves detections from common-envelope evolution with LISA
- Stable mass transfer can explain massive binary black hole mergers with a high spin component
- SCATTER: A New Common Envelope Formalism
- Evolution and final fate of massive post-common-envelope binaries
- The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
- Criteria for Dynamical Timescale Mass Transfer of Metal-poor Intermediate-mass Stars
- Forming merging double compact objects with stable mass transfer
- Post-dynamical inspiral phase of common envelope evolution: Binary orbit evolution and angular momentum transport
- X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
- From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
- A Population of Neutron Star Ultraluminous X-ray Sources with A Helium Star Companion
- Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
- Common origin for black holes in both high mass X-ray binaries and gravitational-wave sources
- The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars
- Whispering in the dark: Faint X-ray emission from black holes with OB star companions
- Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
- Tayler Instability Revisited
- Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
- Development of convective envelopes in massive stars: Implications for gravitational wave sources
- Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
- Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
- Ultraluminous X-ray sources with He star companions
- Wolf-Rayet -- compact object binaries as progenitors of binary compact objects