Hostname: page-component-5b777bbd6c-4n89n Total loading time: 0 Render date: 2025-06-23T06:43:04.241Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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