Probing supermassive black hole binaries with pulsar timing

被引：19
|
作者：
Mingarelli, Chiara M. F. [1 ]
机构：
[1] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA
来源：
NATURE ASTRONOMY | 2019年 / 3卷 / 01期
关键词：
GALACTIC NUCLEI; EVOLUTION;
D O I：
10.1038/s41550-018-0666-y
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The detection of a gravitational-wave background at nanohertz frequencies can tell us if and how supermassive black holes merge, and inform our knowledge of galaxy merger rates and supermassive black hole masses. All we have to do is time pulsars.
引用
收藏
页码：8 / 10
页数：3
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