BLACK HOLES IN BINARIES AND GALACTIC NUCLEI: DIAGNOSTICS, DEMOGRAPHY AND FORMATION
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2001年
关键词:
D O I:
10.1007/10720995_75
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The existence of supermassive collapsed objects in the cores of most galaxies poses still-unanswered questions. First, how did they form, and how does their mass depend on the properties of the host galaxy? Second, can observations probe the metric in the strong-field domain, testing whether it indeed agrees with the Kerr geometry predicted by general relativity (and, if so, what the spin is)?