Parametric dependence of the collinear equilibria and of their stability in the equatorial magnetic-binary problem
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Publication:1111045
DOI10.1007/BF00714159zbMath0657.70014OpenAlexW2071385694MaRDI QIDQ1111045
Publication date: 1988
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf00714159
stabilityequilibrium pointmagnetic-binary systemequatorial magnetic-binary problemmethod of characteristic roots
Related Items (4)
Particle motions around, between or outside the two dipoles of a magnetic binary system ⋮ Charged particles' areas of three-dimensional motions in a system of two magnetic stars ⋮ On the efficiency of Runge-Kutta-Nyström methods with interpolants for solving equations of the form \(Y=F(T,Y,Y')\) over short timespans ⋮ The rotating magnetic-binary problem: A new realistic description of magnetic-binary systems
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