ROSAT HRI catalogue of X-ray sources in the SMC region

被引:50
作者
Sasaki, M [1 ]
Haberl, F [1 ]
Pietsch, W [1 ]
机构
[1] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 2000年 / 147卷 / 01期
关键词
catalogs; galaxies : magellanic clouds; galaxies : stellar content; X-rays : galaxies; X-rays : stars;
D O I
10.1051/aas:2000290
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During the operational phase of the ROSAT satellite between 1990 and 1998 the X-ray telescope pointed 71 times to the Small Magellanic Cloud (SMC) for observations with the High Resolution Imager (HRI), covering a field of 5 degrees x 5 degrees. From these data a catalogue of 121 discrete X-ray sources was derived. By cross-correlating the source catalogue with the SIMBAD data base and the TYCHO catalogue, the systematic positional error of the HRI source positions could be reduced. In total the X-ray position for 99 HRI sources was corrected yielding positional errors between 1 " and 16 ". The HRI catalogue was also cross-correlated with the catalogues derived from the ROSAT Position Sensitive Propotional Counter (PSPC) pointings (Kahabka et al. 1999; Haberl et al. 2000). For 75 HRI sources PSPC counterparts were found and thus hardness ratios are given. With the help of the information obtained from the cross-correlations 56 HRI sources were identified with objects of known or proposed nature. Four foreground stars, six supernova remnants, four supersoft sources, 12 X-ray binaries, and one AGN were detected by the HRI. Based on the existence of a likely optical counterpart or properties like hardness ratio and X-ray to optical flux ratio, further 15 HRI sources were classified into different source types.
引用
收藏
页码:75 / 91
页数:17
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