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On the Tassoul approximation scheme for determining the structure of rotating stars
Published online by Cambridge University Press: 04 August 2017
Extract
The method used by Tassoul and Tassoul assumes a “turbulent viscosity” which is important in determining the dynamics, but is unimportant in heat transport. This approximation is inconsistent, the argument is as follows:
The rotation is expanded about uniform rotation in a series.
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- III. BINARITY, PULSATION, ROTATION AND MIXING
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- Copyright © Reidel 1984