Abstract
The non-radial oscillations of the homogeneous model of a star have been investigated taking into account the variation of the ratio of the specific heats. The stability of the oscillations thus set in is established.
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Bhatia, P.K. Non-radial oscillations of a star. Astrophys Space Sci 166, 219–228 (1990). https://doi.org/10.1007/BF01094895
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DOI: https://doi.org/10.1007/BF01094895