Star Formation by Condensation, I

Details Star Formation by Condensation, I Star Formation by Condensation, I

Jan 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..15..129h&link_type=abstract

Astrophysics and Space Science, Volume 15, Issue 1, pp.129-136

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

We describe two possibilities for the formation of a star by transition of molecular hydrogen from gaseous to the liquid phase in the gravitational field of a spherical mass. Model A.: Contraction through condensation of a polytropic respectively isothermal gas sphere. Model B: Condensation in the isothermal atmosphere which surrounds a core. Model B is sooner possible, because model A introduces certain restrictions of mass and radius of the protostar.

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