The angular resolution of space-based gravitational wave detectors

被引：0
|
作者：
Moore, TA [1 ]
Hellings, RW [1 ]
机构：
[1] Pomona Coll, Dept Phys, Claremont, CA 91711 USA
来源：
GRAVITATIONAL WAVES | 2000年 / 523卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Currently proposed space-based gravitational wave detectors consist of satellite arrays deployed in an equilateral triangle either in the ecliptic plane or in a precessing plane tilted at 60 degrees with respect to the ecliptic. This paper summarizes recent calculations of how well these two types of detectors can resolve the angular positions of two kinds of sources: low-mass compact binary sources and massive-black-hole binaries just before coalescence. Our results show that including higher-order post-Newtonian terms in the gravitational wavefunctions is important when predicting the angular resolution of ecliptic-plane detectors.
引用
收藏
页码：255 / 258
页数：4
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