A unified model for black hole X-ray binary jets?

被引：0
|
作者：
Fender, R [1 ]
Belloni, T
Gallo, E
机构：
[1] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England
[2] Osserv Astron Brera, INAF, I-23807 Merate, Italy
[3] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2005年 / 300卷 / 1-3期
关键词：
accretion; black hole physics; ISM; jets and outflows;
D O I：
10.1007/s10509-005-1201-z
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have recently put forward a 'unified' semi-empirical model for the coupling between accretion and jet production in galactic black hole X-ray binaries. In this paper, we summarise this model and briefly discuss relevant considerations that have arisen since its publication.
引用
收藏
页码：1 / 13
页数：13
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