On the luminosity of spherical protostars

Details On the luminosity of spherical protostars On the luminosity of spherical protostars

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....40..397a&link_type=abstract

Astronomy and Astrophysics, vol. 40, no. 4, May 1975, p. 397-399. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

38

Astronomical Models, Protostars, Stellar Evolution, Stellar Luminosity, Hertzsprung-Russell Diagram, Magnetohydrodynamics, Shock Fronts, Stellar Structure

Scientific paper

Hydrodynamic model computations have been carried out for a spherically symmetric protostar of one solar mass. Compared to similar computations by Larson (1969), different treatment of the accretion shock front is used. The computations basically confirm Larson's results and show that Larson's disputed shock jump conditions have little influence on the protostellar models.

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