Results 191 to 200 of about 385 (218)

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 binaries

Nuclear Physics B - Proceedings Supplements, 2000
P.A. Charles, J.-M. Hameury
openaire   +1 more source

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  

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  

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
J -P Zahn, P North
exaly  

Eccentricity distribution of wide low-mass binaries

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

Gamma-ray binaries and related systems

Astronomy and Astrophysics Review, 2013
Guillaume Dubus, Dubus Guillaume
exaly