Results 191 to 200 of about 403 (217)

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
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X-ray Binaries

1995
Lewin, W.H.G., van Paradijs, J.A., van den Heuvel, E.P.J.   +2 more
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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.
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X-ray binaries

Nuclear Physics B - Proceedings Supplements, 2000
P.A. Charles, J.-M. Hameury
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The eccentricity distribution of wide binaries and their individual measurements

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

Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems

Galaxies, 2022
Tamás Borkovits
exaly  

Variability, periodicity, and contact binaries in WISE

Monthly Notices of the Royal Astronomical Society, 2021
Nadia Zakamska, Matthew Hill, Vedant Chandra   +2 more
exaly  

Frequency of Planets in Binaries

Galaxies, 2020
Silvano Desidera, Mariangela Bonavita
exaly  

X-Ray Binaries

2019
Michael A Nowak, Dominic J Walton
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New low mass ratio contact binaries in the Catalina Sky Survey

Monthly Notices of the Royal Astronomical Society, 2022
Marcio Catelan, Athanasios Papageorgiou, Carlos Eduardo Ferreira Lopes   +2 more
exaly