X-ray fluctuations from locally unstable advection-dominated disks

被引:71
|
作者
Manmoto, T
Takeuchi, M
Mineshige, S
Matsumoto, R
Negoro, H
机构
[1] CHIBA UNIV,FAC SCI,DEPT PHYS,INAGE KU,CHIBA 263,JAPAN
[2] INST SPACE & ASTRONAUT SCI,SAGAMIHARA,KANAGAWA 226,JAPAN
来源
ASTROPHYSICAL JOURNAL | 1996年 / 464卷 / 02期
关键词
accretion; accretion disks; black hole physics; stars; individual (Cygnus X-1); X-rays;
D O I
10.1086/310097
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The response of advection-dominated accretion disks to local disturbances is examined by one-dimensional numerical simulations. It is generally believed that advection-dominated disks are thermally stable. We, however, find that any disturbance added onto accretion flow at large radii does not decay so rapidly that it can move inward with roughly the free-fall velocity. Although disturbances continue to be present, the global disk structure will not be modified greatly. This can account for persistent hard X-ray emission with substantial variations observed in active galactic nuclei and stellar black hole candidates during the hard state. Moreover, when the disturbance reaches the innermost parts, an acoustic wave emerges, propagating outward as a shock wave. The resultant light variation is roughly (time) symmetric and is quite reminiscent of the observed X-ray shots of Cygnus X-1.
引用
收藏
页码:L135 / L138
页数:4
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