Gravitational radiation and spiralling time of close binary systems. III

Details Gravitational radiation and spiralling time of close binary systems. III Gravitational radiation and spiralling time of close binary systems. III

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.167..161p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 167, no. 1, May 1990, p. 161-165.

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Gravitational Waves, Stellar Systems, K Stars, O Stars, Stellar Radiation, Time Dependence

Scientific paper

Twenty-seven typical binary systems have been investigated to study
their power-output by gravitational radiation P(B) and spiralling time
tau(0) relation. It was found that these binary systems form two
distinct groups. New relations are given between P(B) and tau(0) for
each group.

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