Abstract
The oscillations of a polytrope with infinite electric conductivity containing a weak internal poloidal magnetic field which is continuous with an external dipole field are examined with the aid of a variational equation. The corrections to the fundamental characteristic frequencies of the radial and non-radiall=2 pulsation modes are calculated. The magnetic field removes a degeneracy which occurs between these two modes and the resulting frequency splitting is evaluated. The relevance of the results to the known magnetic stars is briefly discussed.
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Fahlman, G.G. The effect of a poloidal magnetic field on the radial and non-radial oscillations of a gaseous mass. Astrophys Space Sci 12, 424–455 (1971). https://doi.org/10.1007/BF00651431
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DOI: https://doi.org/10.1007/BF00651431