The magnetohydrodynamics of stellar structures

Details The magnetohydrodynamics of stellar structures The magnetohydrodynamics of stellar structures

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990japa...11...23d&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 11, March 1990, p. 23-28.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics, Relativity, Stellar Structure, Equations Of State, Formalism, Schwarzschild Metric

Scientific paper

The relativistic magnetofluid equations of stellar structure are derived, assuming that matter is described by perfect magnetofluid. Also, the Schwarzschild solution for homogeneous masses for a vanishing magnetic field h and a magnetized version of the Schwarzschild solution are presented. It is shown that the equation of stellar structure described by an ideal fluid is recovered when the magnetic field h is vanishing.

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