Binary stars as sources of monochromatic gravitational waves

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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Bibliographic Details
Published in:Astronomy reports 2015-06, Vol.59 (6), p.525-541
Main Authors: Vlasov, I. Yu, Sazhina, O. S., Sementsov, V. N., Sazhin, M. V.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Double stars
Gravitational waves
Observations and Techniques
Physics
Physics and Astronomy
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Description
Summary: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).
ISSN:1063-7729
1562-6881
DOI:10.1134/S1063772915060189