Late stages of solar type protostars |
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Authors: | Karl-Heinz A Winkler |
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Institution: | (1) Max-Planck-Institut für Physik und Astrophysik, München, Germany |
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Abstract: | 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.Paper presented at the Conference on Protostars and Planets, held at the Planetary Science Institute, University of Arizona, Tucson, Arizona, between January 3 and 7, 1978. |
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