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

DOI10.1007/s10509-008-9970-9zbMath1172.85302OpenAlexW2061875988MaRDI QIDQ835533

Telemachus J. Kalvouridis

Publication date: 28 August 2009

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

Full work available at URL: https://doi.org/10.1007/s10509-008-9970-9

zbMATH Keywords

systems of magnetic binary starszero-velocity surfaces

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Motions in the field of two rotating magnetic dipoles. III: Zero-velocity curves and surfaces
• Parametric dependence of the collinear equilibria and of their stability in the equatorial magnetic-binary problem
• The symplectic character of orbits in the planar magnetic-binary problem
• The magnetic-binaries problem: Motion of a charged particle in the region of a magnetic-binary system
• Particle motions around, between or outside the two dipoles of a magnetic binary system
• Three-dimensional equilibria and their stability in the magnetic-binary problem
• The symplectic character of the three-dimensional magnetic-binary problem
• Symmetric motions in the Equatorial Magnetic-Binary Problem
• BURRAU'S PROBLEM OF THREE BODIES

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