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X-ray binaries and stellar evolution
Space Science Reviews, 1981Observational evidence suggests that most — if not all — binary X-ray sources are neutron stars. The evolutionary status and possible formation mechanisms of the type I (massive) and type II (low-mass) X-ray binaries are discussed. The difference between the “standard” massive X-ray binaries and the Be/X-ray binaries is ascribed to a somewhat different
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X-ray scattering in x-ray binary pulsars
AIP Conference Proceedings, 1994In x‐ray pulsars, the emission from the bottom of the accretion column in the magnetic pole propagates to the observers through the surrounding environment: the magnetosphere, the accretion disk and the disk corona, the stellar wind, the companion’s atmosphere, and finally the interstellar medium.
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Circumbinary Accretion: From Binary Stars to Massive Binary Black Holes
Annual Review of Astronomy and Astrophysics, 2023Dong Lai, Diego J Munoz
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Nuclear Physics B - Proceedings Supplements, 2000
P.A. Charles, J.-M. Hameury
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P.A. Charles, J.-M. Hameury
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The Evolution of Compact Binary Star Systems
Living Reviews in Relativity, 2014Konstantin Postnov
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The Evolution of Compact Binary Star Systems
Living Reviews in Relativity, 2006Konstantin Postnov
exaly