Late stages of solar type protostars
| Autor: | Karl-Heinz A. Winkler |
|---|---|
| Rok vydání: | 1978 |
| Předmět: |
Physics
Stellar atmosphere Astronomy and Astrophysics Radius Astrophysics law.invention Convection zone Space and Planetary Science law Gravitational collapse Earth and Planetary Sciences (miscellaneous) Radiative transfer Protostar Astrophysics::Earth and Planetary Astrophysics Hydrostatic equilibrium Stellar evolution Astrophysics::Galaxy Astrophysics |
| Zdroj: | The Moon and the Planets. 19:237-244 |
| ISSN: | 1573-0794 0165-0807 |
| Popis: | A consistent hydrodynamical and radiative transfer calculation in spherical symmetry for a 1M ⊙ protostar is presented. The calculation starts with Larson's initial conditions and continues until almost all the material has fallen onto a hydrostatic core with a large outer convection zone. The innermost percent of the mass is partially degenerate. Due to the numerical technique used, the radius of the hydrostatic core is determined with a high degree of accuracy. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|
Full text from SpringerLink