Article contents
A Numerical Investigation of Rotational Instabilities in Differentially Rotating Polytropes
Published online by Cambridge University Press: 25 April 2016
Extract
All studies of circulation in stars have been based on a linear perturbation analysis (e.g. Sung 1975). This analysis establishes criteria for the onset of circulation and, if the perturbations remain weak, allows the circulation pattern to be determined. (For a survey see Tassoul 1978).
- Type
- Contributions
- Information
- Copyright
- Copyright © Astronomical Society of Australia 1980
References
- 4
- Cited by