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Asymptotic Theory of Low-Degree Stellar Acoustic Oscillations
Published online by Cambridge University Press: 12 April 2016
Abstract
We extend the second-order asymptotic description developed by Tassoul (1980, 1990) to the forth order, taking into account both gravity perturbations and realistic (non-polytropic) structure of the stellar envelope. We examine the accuracy of the asymptotic description by the direct computations for a solar model.
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- VI. Asteroseismology: theory
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- Copyright © Astronomical Society of the Pacific 1993
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