The physical approach to the hot star description
Astrophysics
2009-04-19 v9
Abstract
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.
Keywords
Cite
@article{arxiv.0802.1581,
title = {The physical approach to the hot star description},
author = {B. V. Vasiliev},
journal= {arXiv preprint arXiv:0802.1581},
year = {2009}
}