Intermediate-mass black holes in active galactic nuclei

被引：2

作者：

Barth, AJ ^{[1
]}

Greene, JE ^{[1
]}

Ho, LC ^{[1
]}

机构：

[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

来源：

GROWING BLACK HOLES: ACCRETION IN A COSMOLOGICAL CONTEXT | 2005年

关键词：

D O I：

10.1007/11403913_26

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Little is currently known about the demographics of black holes in the intermediate-mass range 10(3) - 10(6) M-circle dot, but a small fraction of dwarf galaxies and late-type spirals contain active nuclei that can be used to study black holes in this mass range. We review the properties of the best-known cases and describe a new project that uses AGNs from the Sloan Digital Sky Survey to extend the M - sigma relation to masses below 10(6) M-circle dot.

引用

页码：154 / 158

页数：5

共 24 条

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