Other
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.216..139p&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 216, Sept. 1, 1985, p. 139-154.
Other
89
Adiabatic Conditions, Magnetic Stars, Stellar Magnetic Fields, Stellar Rotation, Angular Velocity, Gravitational Effects, Magnetic Field Configurations, Stellar Models
Scientific paper
Attention is given to the effect of uniform rotation on the instabilities last discussed by Tayler (1982) and Van Asshe et al. (1982). While rotation exerts some stabilizing influence, it does not seem to remove most instabilities; in some cases, complete stability may be produced at the expense of an unrealistically high rotation speed, while in others the instability growth rate may be reduced while instabilities remain free to grow in times that are very short by comparison with any duration that is important in stellar evolution. All these results are obtained from approximate treatments of the problem, so that they must be seen as less than rigorously established.
Pitts E.
Tayler Roger John
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