Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer -- Application in High Mass X-ray Binaries [PDF]
arXivBinary stars are responsible for many unusual astrophysical phenomena, including some important explosive cosmic events. The stability criteria for rapid mass transfer and common-envelope evolution are fundamental to binary star evolution.
Hongwei Ge +7 more
semanticscholar +9 more sources
Radio emission from colliding outflows in high-mass X-ray binaries with strongly magnetized neutron stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 We present a toy model for radio emission in HMXBs with strongly magnetized NSs where a wind-collision region is formed by the NS outflow and the stellar wind of the massive companion.
Margaritis Chatzis +2 more
semanticscholar +9 more sources
Origin of young accreting neutron stars in high-mass X-ray binaries in supernova remnants [PDF]
Monthly Notices of the Royal Astronomical Society, 2022 Recently, several accreting neutron stars (NSs) in X-ray binary systems inside supernova remnants have been discovered. They represent a puzzle for the standard magneto-rotational evolution of NSs, as their ages (.
A. Khokhriakova, С. Б. Попов
semanticscholar +5 more sources
Determination of wind-fed model parameters of neutron stars in high-mass X-ray binaries [PDF]
Publications of the Astronomical Society of Australia, 2022 We have studied several neutron star high-mass X-ray binaries (HMXBs) with super-giant (SG) companions using a wind-fed binary model associated with the magnetic field.
Ali Taani +4 more
semanticscholar +4 more sources
Evolution of neutron stars in high-mass X-ray binaries [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 We consider the evolution of neutron stars during the X-ray phase of high-mass binaries. Calculationsareperformedassumingacrustal originofthemagneticfield.Astrongwindfrom the companion can significantly influence the magnetic and spin behaviour of a ...
V. Urpin, D. Konenkov, U. Geppert
semanticscholar +4 more sources
Spin evolution of neutron stars in wind-fed high-mass X-ray binaries [PDF]
Publications of the Astronomical Society of Japan, 2020 The observed X-ray pulse period of OB-type high-mass X-ray binary (HMXB) pulsars are typically longer than 100 seconds. It is considered that the interaction between the strong magnetic field of neutron star and the wind matter could cause such a long ...
Shigeyuki Karino
semanticscholar +6 more sources
Multiwavelength Characterization of the High-mass X-Ray Binary Population of M33 [PDF]
Astrophysical Journal, 2023 We present multiwavelength characterization of 65 high-mass X-ray binary (HMXB) candidates in M33. We use the Chandra ACIS survey of M33 (ChASeM33) catalog to select hard X-ray point sources that are spatially coincident with UV-bright point-source ...
M. Lazzarini +14 more
semanticscholar +1 more source
Confirming NGC 6231 as the parent cluster of the runaway high-mass X-ray binary HD 153919/4U 1700-37 with Gaia DR2 [PDF]
Astronomy & Astrophysics, 2021 Context. A significant fraction (10-20%) of the most massive stars move through space with a high (v & 30 km s−1) velocity. One of the possible physical explanations is that a supernova in a compact binary system results in a high recoil velocity of the ...
Vincent van der Meij +3 more
semanticscholar +1 more source
Multiwavelength Characterization of the High-mass X-Ray Binary Population of M31 [PDF]
Astrophysical Journal, 2020 We present our analysis of high-quality high-mass X-ray binary (HMXB) candidates in M31 selected from point-source optical counterpart candidates from the Chandra-PHAT survey catalog.
M. Lazzarini +9 more
semanticscholar +1 more source
Rapid population synthesis of black hole high-mass X-ray binaries: implications for binary stellar evolution [PDF]
Monthly notices of the Royal Astronomical Society, 2023 We conduct binary population synthesis to investigate the formation of wind-fed high-mass X-ray binaries containing black holes (BH-HMXBs). We evolve multiple populations of high-mass binary stars and consider BH-HMXB formation rates, masses, spins ...
I. Romero-Shaw +4 more
semanticscholar +1 more source