Gravitational radiation and spiralling time of close binary systems. IV

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

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185..101p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 185, no. 1, Nov. 1991, p. 101-106.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Eccentric Orbits, Gravitational Waves, Pulsars, Stellar Rotation, Relativistic Theory, Star Formation

Scientific paper

Binary systems with their primary and secondary component masses less than 2 solar masses have been investigated to evaluate the rate of emission of gravitational energy (PB) and spiralling time (tau exp 0) for them. In all, 22 binary systems have been considered. It is found that in spite of the same mass range, these systems form two distinct groups. New relations have been given between PB and tau exp 0 for each group. For a few eccentric orbit systems the rate of decay of orbital periods due to the loss of energy from the system via giavitational radiation emission has also been given and compared with a short-period binary pulsar.

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