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A Numerical Investigation of Rotational Instabilities in Differentially Rotating Polytropes

Published online by Cambridge University Press:  25 April 2016

G. S. Lorimer  and
J. J. Monaghan
G. S. Lorimer
Affiliation:
Department of Mathematics, Monash University
J. J. Monaghan
Affiliation:
Department of Mathematics, Monash University
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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
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 45 - 46
Copyright
Copyright © Astronomical Society of Australia 1980

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References

Gingold, R. A., and Monaghan, J. J., Mon. Not. R. Astron. Soc., 184, 481 (1978).Google Scholar
Gingold, R. A., and Monaghan, J. J., ‘The Roche problem for polytropes in central orbits’, Mon. Not. R. Astron. Soc., (1980). (In Press).CrossRefGoogle Scholar
Hide, R., and Mason, P. J., Adv. Phys., 24, 47 (1975).Google Scholar
Sung, C.-H., Astrophys. and Space Sci., 33, 127 (1975).Google Scholar
Tassoul, J.-L., ‘Theory of Rotating Stars’, pp. 188–218, Princeton University Press, Princeton, New Jersey (1978).Google Scholar