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The core evolution of a globular cluster containing massive black holes
ZHOU, Y; Xie GZ(谢光中)
发表期刊ASTROPHYSICS AND SPACE SCIENCE
1990-06
卷号168期号:2页码:233-241
产权排序第2完成单位
收录类别SCI
摘要This paper considers effects of the general relativity and an accreting black hole in a globular cluster by studying the evolution of a globular cluster core as a whole (i.e., without the partition of the core into the so-called cusp and isothermal core regions). The globular cluster core is assumed to contain a massive black hole at its center. It is shown that the final fate of the evolution of a globular cluster core depends on the mass of the black hole at its center. When the mass M of the black hole is greater than 3000 solar masses, there will be a contraction of the core. On the other hand, if the mass of the black hole is smaller (between 100 and 3000 solar masses) in the center, the core will expand until complete dissolution.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-640X
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WOS记录号WOS:A1990DJ92500008
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/6918
专题星系研究组
通讯作者ZHOU, Y
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GB/T 7714
ZHOU, Y,Xie GZ. The core evolution of a globular cluster containing massive black holes[J]. ASTROPHYSICS AND SPACE SCIENCE,1990,168(2):233-241.
APA ZHOU, Y,&谢光中.(1990).The core evolution of a globular cluster containing massive black holes.ASTROPHYSICS AND SPACE SCIENCE,168(2),233-241.
MLA ZHOU, Y,et al."The core evolution of a globular cluster containing massive black holes".ASTROPHYSICS AND SPACE SCIENCE 168.2(1990):233-241.
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