Volume 455, Number 3, September I 2006
|Page(s)||1165 - 1168|
|Section||Online catalogs and data|
|Published online||16 August 2006|
Catalogue of high-mass X-ray binaries in the Galaxy (4th edition)
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, PR China e-mail: firstname.lastname@example.org
2 Sterrenkundig Instituut “Anton Pannekoek”, Universiteit van Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
Accepted: 18 April 2006
We present a new edition of the catalogue of high-mass X-ray binaries in the Galaxy. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters of the components and other characteristic properties of 114 high-mass X-ray binaries, together with a comprehensive selection of the relevant literature. The aim of this catalogue is to provide the reader with some basic information on the X-ray sources and their counterparts in other wavelength ranges (γ-rays, UV, optical, IR, radio). About 60% of the high-mass X-ray binary candidates are known or suspected Be/X-ray binaries, while 32% are supergiant/X-ray binaries. Some sources, however, are only tentatively identified as high-mass X-ray binaries on the basis of their X-ray properties similar to the known high-mass X-ray binaries. Further identification in other wavelength bands is needed to finally determine the nature of these sources. In cases where there is some doubt about the high-mass nature of the X-ray binary this is mentioned. Literature published before 1 October 2005 has, as far as possible, been taken into account.
Key words: catalogs / X-ray: binaries / stars: emission-line, Be / stars: binaries: general
© ESO, 2006
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