The equatorial equilibrium-configurations of the magnetic-binary problem

Details The equatorial equilibrium-configurations of the magnetic-binary problem The equatorial equilibrium-configurations of the magnetic-binary problem

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cemec..35..397k&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 35, April 1985, p. 397-408.

Statistics

Computation

13

Binary Stars, Equatorial Orbits, Magnetic Stars, Stellar Models, Circular Orbits, Computational Astrophysics, Particle Motion, Variational Principles

Scientific paper

The equatorial motion of a point in the dynamic model of a magnetic binary system developed by Mavraganis (1978) is investigated analytically, with a focus on the equilibrium points (EPs). The locations of the EPs are determined by classical numerical solution of algebraic systems, using zero-velocity-curve EPs as starting points and the stability of these EPs is evaluated in detail on the basis of variational equations for infinitesimal displacements. Numerical results for parameter values similar to those of the earth-sun system are given in tables.

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