Modeling the star formation process. I - Hydrostatic models
Abstract
In the present paper, some of the classical hydrostatic computations carried out by such investigators as Bodenheimer, Hayashi, Larson, Ezer, and Cameron in the 1960s are briefly reviewed. A numerical method for calculating the evolution of protostars is proposed, in which a protostar is treated as an object that has not reached the main sequence.
- Publication:
-
Postepy Astronomii Krakow
- Pub Date:
- June 1979
- Bibcode:
- 1979PoAst..27...73R
- Keywords:
-
- Hydrostatics;
- Protostars;
- Star Formation;
- Stellar Models;
- Astronomical Models;
- Hertzsprung-Russell Diagram;
- Line Spectra;
- Metals;
- Stellar Mass;
- Astrophysics