Partially degenerate nonrelativistic isothermal gas spheres in the presence of a magnetic field

Details Partially degenerate nonrelativistic isothermal gas spheres in the presence of a magnetic field Partially degenerate nonrelativistic isothermal gas spheres in the presence of a magnetic field

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.184...65s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 184, no. 1, Oct. 1991, p. 65-76.

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2

Degenerate Matter, Interstellar Gas, Magnetic Field Configurations, Plasma Equilibrium, Poloidal Flux, Stellar Models, Hydrostatics, Isothermal Processes, Moments Of Inertia, Nonrelativistic Mechanics

Scientific paper

The effect of a weak poloidal magnetic field on the equilibrium structure of a partially degenerate nonrelativistic isothermal gas sphere has been studied. Models have been computed for varying degrees of central degeneracy and the effect of the magnetic field on the various parameters, e.g., mass, central condensation, moment of inertia, and oblateness has been looked into. It is found that as the central degeneracy parameter is increased, the central condensation in general decreases and, hence, the eccentricity of the configuration decreases.

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