Prospects for the detection of electromagnetic counterparts to gravitational wave events

被引：35

作者：

Sylvestre, J ^{[1
]}

机构：

[1] CALTECH, LIGO Lab, Pasadena, CA 91125 USA

来源：

ASTROPHYSICAL JOURNAL | 2003年 / 591卷 / 02期

关键词：

binaries : close; gravitational waves; techniques : miscellaneous;

D O I：

10.1086/375505

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Various models for electromagnetic emissions correlated with the gravitational wave signals expected to be detectable by the current and planned gravitational wave detectors are studied. The position error on the location of a gravitational wave source is estimated and used to show that it could be possible to observe the electromagnetic counterparts to neutron star - neutron star or neutron star - black hole binary coalescences detected with the Advanced Laser Interferometer Gravitational Wave Observatory (LIGO) and the Virgo detectors.

引用

页码：1152 / 1156

页数：5

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