Simulation of the star-formation process. II - Hydrodynamic models

Details Simulation of the star-formation process. II - Hydrodynamic models Simulation of the star-formation process. II - Hydrodynamic models

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979poast..27..165r&link_type=abstract

Postepy Astronomii, vol. 27, July-Sept. 1979, p. 165-184. In Polish.

Other

Hydrodynamics, Protostars, Star Formation, Stellar Models, Cosmic Dust, Gravitational Collapse, Planetary Nebulae, Stellar Envelopes

Scientific paper

The present paper is a continuation of calculations concerning the evolution of a 'protostar'. The term protostar may include any state, starting from unstable gravitation of a molecular cloud to a star of the north polar sequence with a gas-and-dust envelope. One-dimensional (i.e., spherically symmetric) models, two-dimensional (i.e., axially symmetric) models, and three-dimensional (i.e., all other than spherically and axially symmetric) models are analyzed.

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