Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-02-12
Astronomy and Astrophysics
Astrophysics
Scientific paper
The theoretical discription of a hot star interior is obtained. It explains the distribution of stars over their masses, mass-radius-temperature and mass-luminosity dependencies. The theory of the apsidal rotation of binary stars and the spectrum of solar oscillation is considered. All obrained theoretical predictions are in a good agreement with the known measurement data, which confirms the validity of this consideration.
No associations
LandOfFree
The physical approach to the hot star description 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 physical approach to the hot star description, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The physical approach to the hot star description will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-107998