Binary stars as sources of monochromatic gravitational waves

被引：0
|
作者：
I. Yu. Vlasov
O. S. Sazhina
V. N. Sementsov
M. V. Sazhin
机构：
[1] Lomonosov Moscow State University,Sternberg Astronomical Institute
来源：
Astronomy Reports | 2015年 / 59卷
关键词：
Black Hole; Gravitational Wave; Astronomy Report; Quadrupole Moment; Orbital Plane;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Binary stars are considered as possible sources of monochromatic gravitational waves. The amplitude of corrections to the metric generated by such sources is discussed. Three systems that have amplitudes for stresses of the metric exceeding 10−20 are identified (V1182 Aql, V3903 Sgr, and DH Cep).
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收藏
页码：525 / 541
页数：16
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