The convection zone in stars with radiation pressure in the presence of magnetic field

Details The convection zone in stars with radiation pressure in the presence of magnetic field The convection zone in stars with radiation pressure in the presence of magnetic field

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.155..249m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 155, no. 2, May 1989, p. 249-256. Research supported by the Ministry of Sc

Astronomy and Astrophysics

Astrophysics

4

Convection Currents, Radiation Pressure, Stellar Envelopes, Stellar Magnetic Fields, B Stars, Magnetic Field Configurations, Magnetic Flux, Specific Heat, Stellar Evolution, Temperature Gradients

Scientific paper

The effect of a uniform magnetic field on the envelope convection zone of an 8.8-solar-mass star has been studied. The adiabatic exponents Gamma(i) (i = 1,2,3), adiabatic temperature gradient, and specific heat of stellar matter have been computed. It is shown that the magnetic field tends to increase the values of adiabatic temperature gradient and specific heats of stellar matter in the envelope convection zone.

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