Abstract
The existence of the point of bifurcation of rotating gaseous masses with toroidal magnetic fields is established from the first variations of the integral properties provided by the second-order virial relations. It is shown that the point of bifurcation, where the Jabcobi ellipsoids branch off from the Maclaurin spheroids, is unaffected by the presence of toroidal magnetic fields.
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Trehan, S.K., Singh, M. The oscillations and the stability of rotating masses with magnetic fields. Astrophys Space Sci 33, 43–48 (1975). https://doi.org/10.1007/BF00646007
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DOI: https://doi.org/10.1007/BF00646007