Radio and X-ray signatures of merging neutron stars

被引：196

作者：

Hansen, BMS ^{[1
]}

Lyutikov, M ^{[1
]}

机构：

[1] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2001年 / 322卷 / 04期

关键词：

gravitation; stars : magnetic fields; stars : neutron; pulsars : general; gamma-rays : bursts; X-rays : bursts;

D O I：

10.1046/j.1365-8711.2001.04103.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe the possible electromagnetic signals expected from the magnetospheric interactions of a neutron star binary prior to merger. We find that both radio and X-ray signals of detectable strength are possible. We discuss possible links with the phenomenon of gamma-ray bursts (GRBs) and describe the prospects for direct detection of these signals in searches for radio and X-ray transients.

引用

页码：695 / 701

页数：7

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