Making accretion disks around black holes: GRB progenitors

被引：0
|
作者：
Fryer, CL [1 ]
Zhang, WQ [1 ]
机构：
[1] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
来源：
GAMMA-RAY BURSTS | 2000年 / 526卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We review the current progenitors of the rapidly accreting black holes which are thought to power gamma-ray bursts. Differences in the evolutionary scenarios of these progenitors lead to differences in the observed properties of the bursts (e.g., burst duration, burst location, and afterglow emission). We pay particular attention to the differences between helium merger and collapsar gamma-ray burst progenitors (the two leading progenitors for long-duration gamma-ray bursts).
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收藏
页码：643 / 647
页数：5
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