A note on the linear stellar model
Abstract
For a purely gaseous self-gravitating stellar configuration with linear matter density distribution the total power generated by nuclear reactions is considered. The analytic connection between physical parameters of the macroscopic and microscopic levels of the stellar equilibrium configuration is revealed.
- Publication:
-
Astronomische Nachrichten
- Pub Date:
- 1987
- DOI:
- 10.1002/asna.2113080506
- Bibcode:
- 1987AN....308..313A
- Keywords:
-
- Density Distribution;
- Stellar Models;
- Stellar Physics;
- Stellar Structure;
- Nuclear Reactions;
- Stellar Evolution;
- Thermodynamic Equilibrium;
- Astrophysics