Numerical models of the formation of the solar nebula

Details Numerical models of the formation of the solar nebula Numerical models of the formation of the solar nebula

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26....8b&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, no. 3, May-June 1992, p. 8-13. In Russian.

Astronomy and Astrophysics

Astronomy

Protostars, Solar Corona, Solar System Evolution, Stellar Evolution, Digital Simulation, Stellar Cores, Stellar Mass, Stellar Temperature

Scientific paper

A new numerical code has been developed for investigating the radiative hydrodynamics of protostar formation. This paper describes recent results of two ongoing projects considering the formation of the solar nebula: (1) the determination of initial conditions leading to single protostellar objects and (2) the calculation of physical conditions in the nebula formed by collapse of a solar mass onto the protostellar core.

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