X-rays from quiescent low-mass X-ray binary transients

被引:0
作者
Lasota, JP [1 ]
机构
[1] Inst Astrophys, F-75014 Paris, France
关键词
stars : binaries : close; accretion; accretion disks; instabilities; X-rays : general;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I argue that it is very unlikely that X-rays from quiescent black-hole low-mass X-ray binary transients are emitted by coronae of companion stars. I show that in a simple model in which these X-rays are emitted by an ADAF filling the inner part of an unsteady, dwarf-nova type disc, the X-ray luminosity is correlated with the orbital period. I predict what values of X-ray luminosities from black-hole transient systems should be observed by Chandra and XMM-Newton.
引用
收藏
页码:575 / 582
页数:8
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