The importance of rapid black hole spin in relativistic jet formation

被引：0
|
作者：
Meier, DL [1 ]
Koide, S [1 ]
机构：
[1] CALTECH, Jet Propuls Lab, Pasadena, CA 91109 USA
来源：
BLACK HOLES IN BINARIES AND GALACTIC NUCLEI: DIAGNOSTICS, DEMOGRAPHY AND FORMATION | 2001年
关键词：
D O I：
10.1007/10720995_44
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a summary of several recent papers on the simulation of relativistic jet formation in the vicinity of rotating and non-rotating black holes. We find that the strongest and fastest jets (Gamma similar to 3) occur when the hole is rotating and the disk plunges rapidly into the ergosphere.
引用
收藏
页码：216 / 217
页数：2
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