Gravitational radiation and spiralling time of close binary systems

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

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137..191p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 1, Oct. 1987, p. 191-194.

Statistics

Computation

4

Eclipsing Binary Stars, Gravitational Waves, Stellar Gravitation, Stellar Orbits, Time Dependence, Computational Astrophysics, Stellar Mass

Scientific paper

Values for the spiral time and power output by gravitational radiation have obtained for 16 close eclipsing binary systems. A predominantly inverse relation between power output and spiralling time is found, with the system with maximum power output having the shortest spiralling time, or being the one that should be the first to collapse. The gravitational radiation/spiral time relation provides a means of cataloguing these systems, and its consequences for the interpretation of these systems are considered.

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