Formation of solar-type stars in spherical symmetry. II - Effects of detailed constitutive relations

Details Formation of solar-type stars in spherical symmetry. II - Effects of detailed constitutive relations Formation of solar-type stars in spherical symmetry. II - Effects of detailed constitutive relations

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..311w&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, May 15, 1980, p. 311-325. Research sponsored by the U.S. Department of Energy.

Astronomy and Astrophysics

Astrophysics

72

Gravitational Collapse, Interstellar Gas, Stellar Evolution, Stellar Mass Accretion, Equations Of State, Hydrodynamic Equations, Ionized Gases, Stellar Envelopes, Stellar Structure, Thermodynamic Properties

Scientific paper

The paper discusses the effects of the evolution of the use of realistic
constitutive relations for formation of solar-type stars in spherical
symmetry. The basic physical assumptions and equations employed are
given. The effects of the detailed equation of state and opacities used
in calculation are analyzed.

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