Results 241 to 250 of about 8,299 (260)

X-ray binaries and stellar evolution

Space Science Reviews, 1981
Observational 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
openaire   +1 more source

X-ray Binaries

1995
Lewin, W.H.G., van Paradijs, J.A., van den Heuvel, E.P.J.   +2 more
openaire   +5 more sources

X-ray scattering in x-ray binary pulsars

AIP Conference Proceedings, 1994
In 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.
openaire   +1 more source

X-ray binaries

Nuclear Physics B - Proceedings Supplements, 2000
P.A. Charles, J.-M. Hameury
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New low mass ratio contact binaries in the Catalina Sky Survey

Monthly Notices of the Royal Astronomical Society, 2022
Panagiota-Eleftheria Christopoulou, Eleni Lalounta, A Papageorgiou   +2 more
exaly  

The eccentricity distribution of wide binaries and their individual measurements

Monthly Notices of the Royal Astronomical Society, 2022
Hsiang-Chih Hwang, Yuan-Sen Ting, Nadia L Zakamska   +2 more
exaly  

X-Ray Binaries

2019
Michael A Nowak, Dominic J Walton
openaire   +1 more source

Gravitational Waves from Merging Compact Binaries

Annual Review of Astronomy and Astrophysics, 2009
Scott A Hughes
exaly  

Circularization in B-type eclipsing binaries in both Magellanic Clouds

New Astronomy Reviews, 2004
P North, J -P Zahn
exaly  

Eccentricity distribution of wide low-mass binaries

Monthly Notices of the Royal Astronomical Society, 2020
Andrei Tokovinin
exaly