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Rotational Perturbation of A Radial Oscillation in A Gaseous Star

Published online by Cambridge University Press:  12 April 2016

R. Simon*
Affiliation:
Institut d’Astrophysique de l’Université de Liège, Cointe-Sclessin, Belgium

Extract

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The perturbation method has been applied to the problem of the oscillations of a gaseous star rotating around a fixed z-axis according to a general law of the type

Type
Part I / The Effects of Rotation on Stellar Interiors and Evolution
Copyright
Copyright © Reidel 1970

References

Simon, R.: 1969, Astron. Astrophys. 2, 390.Google Scholar