XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence

被引：41

作者：

Homan, J

Wijnands, R

Kong, A

Miller, JM

Rossi, S

Belloni, T

Lewin, WHG

机构：

[1] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA

[2] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands

[3] Univ Michigan, Ann Arbor, MI 48109 USA

[4] INAF, Osservatorio Astron Brera, I-23807 Merate, LC, Italy

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2006年 / 366卷 / 01期

关键词：

stars : individual : XTE J1650-500; X-rays : stars;

D O I：

10.1111/J.1365-2966.2005.09843.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the result of an XMM-Newton observation of the black hole X-ray transient XTE J1650-500 in quiescence. The source was not detected, and we set upper limits on the 0.5-10 keV luminosity of 0.9-1.0 x 10(31) erg s(-1) (for a newly derived distance of 2.6 kpc). These limits are in line with the quiescent luminosities of black hole X-ray binaries with similar orbital periods (similar to 7-8 h).

引用

页码：235 / 237

页数：3

共 26 条

[21] State transitions in the 2001/2002 outburst of XTE J1650-500 [J].