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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

Ian W. Roxburgh
Ian W. Roxburgh*
Affiliation:
Department of Applied Mathematics, Queen Mary College, London

Extract

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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.

Type
III. BINARITY, PULSATION, ROTATION AND MIXING
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 517 - 518
Copyright
Copyright © Reidel 1984