Regularization of the equatorial magnetic-binary problem

Details Regularization of the equatorial magnetic-binary problem Regularization of the equatorial magnetic-binary problem

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.120..205m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 120, no. 2, March 1986, p. 205-210.

Statistics

Computation

1

Binary Stars, Computational Astrophysics, Magnetic Stars, Particle Motion, Differential Equations

Scientific paper

The differential equations which describe the equatorial motion of a particle in a magnetic-binary system are regularized by a transformation of the dependent and independent variables. The new equations of motion, which are simpler than the original ones, with only linear velocity and acceleration terms occurring, show the invariant form of the law of motion. Finally, the distinction between the zero-velocity curves and the isotachs in the transformed space is also discussed.

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