Relativistic Magnetic Partially Degenerate Isothermal Gas Spheres

Details Relativistic Magnetic Partially Degenerate Isothermal Gas Spheres Relativistic Magnetic Partially Degenerate Isothermal Gas Spheres

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.184..143p&link_type=abstract

Astrophysics and Space Science, Volume 184, Issue 1, pp.143-146

Astronomy and Astrophysics

Astrophysics

Scientific paper

The effect of a poloidal magnetic field on the structure of isothermal gas spheres in hydrostatic equilibrium under the pressure of partially degenerate relativistic electrons and radiation has been considered. An equation of state involving Fermi-Dirac functionsF 2(ψ) andF 3(ψ) has been used. Modifications to the values of various structural parameters have been tabulated for the cases ψ c =0, 2, 3, 5, and 10, ψ c being the central degeneracy parameter.

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