Galactic X-ray binary jets

被引：0
作者：
Gallo, Elena [1 ]
机构：
[1] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2007年 / 311卷 / 1-3期
关键词：
X-rays : binaries; radiation mechanisms : general; stars : individual (A0620-00);
D O I：
10.1007/s10509-007-9571-z
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
With their relatively fast variability time-scales, Galactic X-ray binaries provide an excellent laboratory to explore the physics of accretion and related phenomena, most notably outflows, over different regimes. After comparing the phenomenology of jets in black hole systems to that of neutron stars, here I discuss the role of the jet at very low Eddington ratios, and present preliminary results obtained by fitting the broadband spectral energy distribution of a quiescent black hole binary with a 'maximally jet-dominated' model.
引用
收藏
页码：161 / 165
页数：5
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