Rotating, post-Newtonian near-ellipsoidal configurations of a magnetized homogeneous fluid

Details Rotating, post-Newtonian near-ellipsoidal configurations of a magnetized homogeneous fluid Rotating, post-Newtonian near-ellipsoidal configurations of a magnetized homogeneous fluid

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59..476t&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, May-June 1982, p. 476-482.) Soviet Astronomy, vol. 26, May-June 1982, p. 289-292. Translati

Astronomy and Astrophysics

Astronomy

Elliptical Plasmas, Neutron Stars, Rotating Plasmas, Gravitational Waves, Magnetohydrodynamic Stability, Magnetohydrostatics, Plasma Equilibrium, Plasma Oscillations, Plasma Potentials, Plasma-Electromagnetic Interaction, Relativity, Stellar Gravitation, Stellar Magnetic Fields, Stellar Models, Stellar Rotation

Scientific paper

A method is developed for determining the figures of equilibrium of rapidly rotating, gravitating, homogeneous fluid bodies, on the assumption that effects tending to deflect the configuration from an ellipsoid are small. The gravitational potential of an arbitrarily perturbed ellipsoid is calculated to the accuracy required, and a system of equations is obtained for the coefficients that occur in the equation of the bounding surface.

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