On the Ratio of Masses Radii Temperatures and Luminosities of the Eclipsing Stars of the Main Sequence Systems

Details On the Ratio of Masses Radii Temperatures and Luminosities of the Eclipsing Stars of the Main Sequence Systems On the Ratio of Masses Radii Temperatures and Luminosities of the Eclipsing Stars of the Main Sequence Systems

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1528...13k&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1528/MAY, P. 13, 1988

Other

Scientific paper

It is shown that in main sequence (MS) eclipsing binary systems with period change (Q ≠ 0), the masses, radii, temperatures and luminosities of the main and companion stars are directly proportional. These stars have the value of the mass ratio q = 0.87+0.03. For other MS systems with Q = 0, these characteristics are related by a power law with a smaller correlation coefficient.

Affiliated with

Also associated with

No associations

Rating

On the Ratio of Masses Radii Temperatures and Luminosities of the Eclipsing Stars of the Main Sequence Systems 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 On the Ratio of Masses Radii Temperatures and Luminosities of the Eclipsing Stars of the Main Sequence Systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Ratio of Masses Radii Temperatures and Luminosities of the Eclipsing Stars of the Main Sequence Systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-854220