Intermediate-mass black holes as LISA sources

被引：33
|
作者：
Miller, M. Coleman [1 ,2 ]
机构：
[1] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[2] Univ Maryland, Maryland Astron Ctr Theory & Computat, College Pk, MD 20742 USA
来源：
CLASSICAL AND QUANTUM GRAVITY | 2009年 / 26卷 / 09期
关键词：
DENSE STAR-CLUSTERS; SPACE-TELESCOPE EVIDENCE; X-RAY SOURCES; GLOBULAR-CLUSTERS; ACCRETION DISKS; GALACTIC-CENTER; MERGERS; GROWTH; GALAXIES; IMBH;
D O I：
10.1088/0264-9381/26/9/094031
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Intermediate-mass black holes (IMBHs), with masses in the range similar to 10(2-4)M(circle dot), would be unique sources of gravitational waves for LISA. Here we discuss their context as well as specific characteristics of IMBH-IMBH and IMBH-supermassive black hole mergers and how these would allow sensitive tests of the predictions of general relativity in strong gravity.
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页数：6
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