The angular momentum of eclipsing binaries

Details The angular momentum of eclipsing binaries The angular momentum of eclipsing binaries

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..94..165s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 94, no. 1, July 1983, p. 165-170.

Astronomy and Astrophysics

Astrophysics

4

Angular Momentum, Eclipsing Binary Stars, Mass Ratios, Stellar Mass, Cosmology, Least Squares Method

Scientific paper

An observational diagram for eclipsing binary systems is presented in order to provide fundamental data for a relationship between the angular momenta (J) and the mass (M). J is quantified for a circular orbit and relations are defined among the orbital radii relative to the gravity center, the components' masses, the total mass, and the mass ratio. An equation is described and used to obtain the J value for 1048 eclipsing binaries, and J-M diagrams are generated for detached, semi-detached, and contact systems. A slope for the three systems clusters around 1.92. Further applications of the diagrams to the local supercluster and the metagalaxy demonstrate that a universal cosmogonic mechanism may exist, which was predicted by the cosmological principle of a hadronic fireball.

Affiliated with

Also associated with

No associations

Rating

The angular momentum of eclipsing binaries 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 The angular momentum of eclipsing binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The angular momentum of eclipsing binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1626869