Catalogue of high-mass X-ray binaries in the Galaxy (4th edition)

被引:338
作者
Liu, Q. Z. [1 ]
van Paradijs, J.
van den Heuvel, E. P. J.
机构
[1] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
[2] Univ Amsterdam, Sterrenkundig Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
关键词
catalogs; X-ray : binaries; stars; emission-line; Be; stars : binaries : general;
D O I
10.1051/0004-6361:20064987
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:1165 / 1168
页数:4
相关论文
共 53 条
[1]   The first IBIS/ISGRI soft gamma-ray Galactic Plane survey catalog [J].
Bird, AJ ;
Barlow, EJ ;
Bassani, L ;
Bazzano, A ;
Bodaghee, A ;
Capitanio, F ;
Cocchi, M ;
Del Santo, M ;
Dean, AJ ;
Hill, AB ;
Lebrun, F ;
Malaguti, G ;
Malizia, A ;
Much, R ;
Shaw, SE ;
Stephen, JB ;
Terrier, R ;
Ubertini, P ;
Walter, R .
ASTROPHYSICAL JOURNAL, 2004, 607 (01) :L33-L37
[2]   A NEW 60 MILLISECOND X-RAY PULSAR AND ITS MASSIVE EARLY-TYPE COMPANION [J].
CARAVEO, PA ;
BIGNAMI, GF ;
GOLDWURM, A .
ASTROPHYSICAL JOURNAL, 1989, 338 (01) :338-&
[3]   Optical and near-infrared observations of the microquasar V4641 Sgr during the 1999 September outburst [J].
Chaty, S ;
Charles, PA ;
Martí, J ;
Mirabel, IF ;
Rodríguez, LF ;
Shahbaz, T .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 343 (01) :169-174
[4]  
CLARK GW, 1975, IAUC, P2843
[5]  
Coe M. J., 2000, ASPC, V214, P656, DOI DOI 10.48550/ARXIV.ASTRO-PH/9911272
[6]   Discovery of the optical counterpart to the ASCA transient AX1845.0-0433 [J].
Coe, MJ ;
Fabregat, J ;
Negueruela, I ;
Roche, P ;
Steele, IA .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1996, 281 (01) :333-338
[7]  
Gotthelf EV, 1998, NEW ASTRON, V3, P293, DOI 10.1016/S1384-1076(98)00014-1
[8]   High-mass X-ray binaries as a star formation rate indicator in distant galaxies [J].
Grimm, HJ ;
Gilfanov, M ;
Sunyaev, R .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 339 (03) :793-809
[9]   A possible X-ray and radio counterpart of the high-energy gamma-ray source 3EG J2227+6122 [J].
Halpern, JP ;
Gotthelf, EV ;
Leighly, KM ;
Helfand, DJ .
ASTROPHYSICAL JOURNAL, 2001, 547 (01) :323-333
[10]  
HALPERN JP, 2004, ATEL, P289