Catalogue of high-mass X-ray binaries in the Galaxy (4th edition)
Catalogue of high-mass X-ray binaries in the Galaxy (4th edition)
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DOI：
10.1051/0004-6361:20064987
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发表时间：
2006-09
影响因子：
3.7
通讯作者：
Q. Z. Liu;J. Paradijs;Edward P. J. van den Heuvel
中科院分区：
文献类型：
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作者：
Q. Z. Liu;J. Paradijs;Edward P. J. van den Heuvel
我们介绍了银河系中高质量X射线二进制文件的新版本。该目录包含源名称，坐标，查找图表，X射线光度，系统参数和组件的恒星参数以及114个高质量X射线二进制文件的其他特性属性，以及相关文献的全面选择。该目录的目的是为读者提供有关X射线源及其其他波长范围（伽马射线，紫外线，光学，IR，无线电）的一些基本信息。大约60％的高质量X射线二进制候选者是/X射线二进制的，而32％是超级/X射线二进制文件。但是，某些来源仅根据与已知的高质量X射线二进制文件相似的X射线特性，初步鉴定为高质量X射线二进制。需要在其他波长频段中进行进一步识别，以最终确定这些源的性质。如果对X射线二进制的高质量性质有疑问，请提及。 2005年10月1日之前发表的文献已被考虑在内。
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 (gamma-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.