Relativistic jets from black hole binaries

被引：0
|
作者：
Corbel, Stephane [1 ,2 ]
机构：
[1] Univ Paris 07, F-91191 Gif Sur Yvette, France
[2] CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, France
来源：
ADVANCES IN SPACE RESEARCH | 2006年 / 38卷 / 12期
关键词：
black hole physics; radio continuum; stars; ISM; jets and outflows;
D O I：
暂无
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Relativistic jets are now believed to be a fairly ubiquitous property of accreting compact objects, and are intimately coupled with the accretion history. Associated with rapid changes in the accretion states of the binary systems, ejections of relativistic plasma can be observed at radio frequencies on timescale of weeks before becoming undetectable. However, recent observations point to long term effects of these ejecta on the interstellar medium with the formation of large scale relativistic jets around binary systems. (C) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：2867 / 2871
页数：5
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