Abstract
The equilibrium general magnetic field inside a magneto-rotating star, assumed to be a polytrope, has been determined more accurately, for large general magnetic field. Furthermore the effect of such field on the structure and oscillations of a slowly rotating polytrope has been studied forn=1,0, 1.5, 2.0, and 3.0.
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Das, M.K., Tandon, J.N. On a uniformly rotating magnetic polytrope. Astrophys Space Sci 49, 261–275 (1977). https://doi.org/10.1007/BF00641980
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DOI: https://doi.org/10.1007/BF00641980