Gravitational radiation and spiralling time of close binary systems (V)

Details Gravitational radiation and spiralling time of close binary systems (V) Gravitational radiation and spiralling time of close binary systems (V)

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.202...63p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 202, no. 1, p. 63-68.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Stellar Gravitation, Stellar Orbits, Stellar Radiation, Stellar Mass, Stellar Systems

Scientific paper

Forty-six binary systems with their primary component masses between 2 and 3 solar masses have been considered for gravitational radiation study. Power output by gravitational radiation (PB) and spiral time tau(0) for all individual systems have been evaluated. A relation has been given between PB and tau(0). The rate of decrease of orbital period has also been given for 10 eccentric orbit systems.

Affiliated with

Also associated with

No associations

Rating

Gravitational radiation and spiralling time of close binary systems (V) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gravitational radiation and spiralling time of close binary systems (V), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational radiation and spiralling time of close binary systems (V) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1369353