Abstract
Perturbation theory is developed for calculating the influence of slow differential rotation on the adiabatic nonradial modes of stellar oscillations. The effects of Coriolis forces and ellipticity are analysed simultaneously using the perturbation technique for Hermitian operators which is developed up to second order in eigenvalues and to first order in eigenvectors.
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Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.
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Vorontsov, S.V. Adiabatic oscillations of a differentially-rotating star. Sol Phys 82, 379–382 (1983). https://doi.org/10.1007/BF00145576
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DOI: https://doi.org/10.1007/BF00145576