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Be–X-ray binaries and candidates

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jun 2005Embargo end date: 01 Jan 2005 English Publisher:Informa UK LimitedJournal:Astronomical & Astrophysical Transactions, volume 24, pages 151-185 (issn: 1055-6796, eissn: 1476-3540,

Authors: N. V. Raguzova; Sergei Popov;

doi: 10.1080/10556790500497311 , 10.48550/arxiv.astro-ph/0505275

arXiv: http://arxiv.org/abs/astro-ph/0505275

Be–X-ray binaries and candidates

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Abstract

We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 130 sources and provides information on names and spectral types of optical components, distances, spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. We give brief comments on each object and provide necessary references to original data.

20 pages, 4 figures, few references added and corrected

Related Organizations

Sternberg Astronomical Institute
Russian Federation

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	83
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 10%

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Top 10%

Green

bronze

Fields of Science

Fields of Science

Related to Research communities

NEANIAS Space Research Community