Roche model analysis of the eclipsing binaries ST Car and RY Ind

Details Roche model analysis of the eclipsing binaries ST Car and RY Ind Roche model analysis of the eclipsing binaries ST Car and RY Ind

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cha%26a..12..106z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 12, Issue 2, p. 106-109.

Astronomy and Astrophysics

Astrophysics

1

Stars, Eclipsing Binaries, Roche Model

Scientific paper

The authors use the Wilson-Devinney Roche model to re-analyse the light curves of two short-period eclipsing binaries, ST Car and RY Ind. The results show that for ST Car, the photometric mass ratio is q ≈ 0.50, and that both are detached systems with the less massive components almost filling their Roche lobes. Their photometric features indicate that they are probably after the Algol stage in their evolution.

Affiliated with

Also associated with

No associations

Rating

Roche model analysis of the eclipsing binaries ST Car and RY Ind 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 Roche model analysis of the eclipsing binaries ST Car and RY Ind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Roche model analysis of the eclipsing binaries ST Car and RY Ind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1180435