DETECTABILITY OF THE GRAVITATIONAL-WAVE SIGNAL FROM A CLOSE NEUTRON-STAR BINARY WITH MASS-TRANSFER

被引：23

作者：

JARANOWSKI, P ^{[1
]}

KROLAK, A ^{[1
]}

机构：

[1] POLISH ACAD SCI,INST MATH,PL-00950 WARSAW,POLAND

来源：

ASTROPHYSICAL JOURNAL | 1992年 / 394卷 / 02期

关键词：

BINARIES; CLOSE; RADIATION MECHANISMS; GRAVITATIONAL; STARS; NEUTRON; TECHNIQUES; INTERFEROMETRIC;

D O I：

10.1086/171610

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Simple analytical models of a neutron star binary with stable mass transfer are constructed. The detectability of the gravitational wave signal from such a system by long-arm laser interferometers is investigated.

引用

页码：586 / 591

页数：6

共 16 条

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