State transitions in the 2001/2002 outburst of XTE J1650-500

被引:18
作者
Rossi, S
Homan, J
Miller, JM
Belloni, T
机构
[1] Astron Observ Brera Merate, INAF, I-23807 Merate, LC, Italy
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
D O I
10.1016/j.nuclphysbps.2004.04.075
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We present a study of the X-ray transient and black hole candidate XTE J1650-500 during its 2001/2002 outburst. The source made two state transitions between the hard and soft states, at luminosity levels that differ by a factor of similar to5-10. The first transition, between hard and soft, lasted for similar to30 days and showed two parts; one part in which the spectral properties evolve smoothly away from the hard state and another that we identify as the,steep power law state'. The two parts showed different behavior of the Fe K emission line and QPO frequencies. The second transition, from soft to hard, lasted only similar to15 days and showed no evidence of the presence of the,steep power law state'. Comparing observations from the early rise and the decay of the outburst, we conclude that the source can be in the hard state in a range of more than 10(4) in luminosity. We briefly discuss the state transitions in the framework of a two-flow model.
引用
收藏
页码:416 / 419
页数:4
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