The physical approach to the hot star description
B.V.Vasiliev
TL;DR
This paper presents a theoretical model of hot star interiors that explains various stellar properties and phenomena, with predictions aligning well with observational data, thereby validating the approach.
Contribution
It introduces a comprehensive physical theory for hot star interiors, linking mass, radius, temperature, luminosity, and stellar oscillations, validated by empirical data.
Findings
Theoretical predictions match observational data.
Explains mass distribution and stellar dependencies.
Describes apsidal rotation and solar oscillations.
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.
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research