Particle motions around, between or outside the two dipoles of a magnetic binary system

DOI10.1007/BF00627780zbMath0803.70003MaRDI QIDQ1331349

Telemachus J. Kalvouridis

Publication date: 2 January 1995

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

influence of oblatenesssymmetric motions

Mathematics Subject Classification ID

Dynamics of a system of particles, including celestial mechanics (70F99) Motion of charged particles (78A35)

Related Items (1)

Charged particles' areas of three-dimensional motions in a system of two magnetic stars

Cites Work

• Unnamed Item
• An application of the scaled Runge-Kutta algorithms to some problems of celestial mechanics
• Parametric dependence of the collinear equilibria and of their stability in the equatorial magnetic-binary problem
• Equilibrium points in the planar magnetic-binary problem
• The symplectic character of orbits in the planar magnetic-binary problem
• Three-dimensional equilibria and their stability in the magnetic-binary problem
• Symmetric motions in the Equatorial Magnetic-Binary Problem
• [https://portal.mardi4nfdi.de/wiki/Publication:3796824 La periodicit� et la symetrie du mouvement equatorial au probl�me magnetique-binaire]
• The equilibrium state in the Magnetic-Binary problem when the more massive primary is an oblate spheroid
• BURRAU'S PROBLEM OF THREE BODIES

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