Evolution of hard X-ray spectra along the branches in Circinus X-1

被引:14
作者
Ding, GQ [1 ]
Qu, JL
Li, TP
机构
[1] Chinese Acad Sci, Inst High Energy Phys, Ctr Particle Astrophys, Beijing 100039, Peoples R China
[2] Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China
[3] Tsing Hua Univ, Dept Phys, Beijing 100084, Peoples R China
[4] Tsing Hua Univ, Ctr Astrophys, Beijing 100084, Peoples R China
基金
中国国家自然科学基金;
关键词
binaries : general; stars : individual (Circinus X-1); X-rays : binaries; X-rays : general; X-rays : individual (Circinus X-1);
D O I
10.1086/379338
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using the data from the Proportional Counter Array and the High-Energy X-Ray Timing Experiment on board the Rossi X-Ray Timing Explorer satellite, we investigate the evolution of the 3-200 keV spectra of the peculiar low-mass X-ray binary Circinus X-1 along the branches on its hardness-intensity diagram (HID) from the vertical horizontal branch, through the horizontal horizontal branch and normal branch, to the flaring branch. We detect a power-law hard component in the spectra. It is found that the derived photon indices (Gamma) of the power-law hard component are correlated with the position on the HID. The power-law component dominates the X-ray emission of Cir X-1 in the energy band higher than similar to 20 keV. The fluxes of the power-law component are compared with those of the bremsstrahlung component in the spectra. A possible origin of the power-law hard component is discussed.
引用
收藏
页码:L219 / L222
页数:4
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