Gravitational radiation and spiralling time of close binary systems. II

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

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..379p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 2, Nov. 1988, p. 379-382.

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Gravitational Waves, Stellar Systems, Eclipsing Binary Stars, Time Functions

Scientific paper

Power-output by gravitational radiation (PB) and spiralling
time (τ0) for individual systems of twelve early (B) type
binary systems have been evaluated. A new relation between PB
and τ0 has been obtained. It is found that most of these
systems lie in the spiralling time range ≡109years.

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