Possible observational tests for some aspects of binary-star evolution theory

Details Possible observational tests for some aspects of binary-star evolution theory Possible observational tests for some aspects of binary-star evolution theory

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1..227k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, Nov. 1975, p. 32-37.) Soviet Astronomy Letters, vol. 1, Nov.-Dec. 1975, p. 227-229.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Binary Stars, Orbit Calculation, Stellar Evolution, Hertzsprung-Russell Diagram, Hot Stars, Schwarzschild Metric, Supergiant Stars, Tables (Data), Visual Observation

Scientific paper

Evolutionary calculations for massive close binary systems are performed using the Schwarzschild criterion for convective stability in the zone of variable molecular weight. The calculations are compared with others that were performed using the Ledoux criterion. Based on this comparison, possibilities are pointed out for the observational verification of the correctness of these criteria.

Affiliated with

Also associated with

No associations

Rating

Possible observational tests for some aspects of binary-star evolution theory 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 Possible observational tests for some aspects of binary-star evolution theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possible observational tests for some aspects of binary-star evolution theory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1579110