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Areas of equatorial motion in the magnetic-binary problem

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Abstract

In the process of modelling the Magnetic-Binary systems, we deal with the permissible areas of motion in the equatorial planes of the representative model. The zero velocity curves, derived by the well known steepest descent method, provide the means for determining these areas. Further these curves reveal all the equilibrium points located on the above planes.

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References

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Authors and Affiliations

  1. Dept. of Mechanics, National Tech. Univ. of Athens, Greece

    T. Kalvoridis, A. Mavraganis & C. Pangalos

  2. Dept. of Mathematics, Patras University, Greece

    Ch. Zagouras

Authors
  1. T. Kalvoridis
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  2. A. Mavraganis
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  3. C. Pangalos
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  4. Ch. Zagouras
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Kalvoridis, T., Mavraganis, A., Pangalos, C. et al. Areas of equatorial motion in the magnetic-binary problem. Celestial Mechanics 37, 161–170 (1985). https://doi.org/10.1007/BF01230925

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  • DOI: https://doi.org/10.1007/BF01230925

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