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Non-Radial Oscillations in Rotating White Dwarfs

Published online by Cambridge University Press:  12 April 2016

J. Papaloizou  and
J.E. Pringle
J. Papaloizou
Affiliation:
Institute of Astronomy, Madingley Rd., Cambridge CB3 OHA
J.E. Pringle
Affiliation:
Institute of Astronomy, Madingley Rd., Cambridge CB3 OHA

Extract

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In previous work (Papaloizou and Pringle, 1978), we investigated analytically the low frequency spectrum of a rotating pulsating star, taking the effects of rotation fully into account. In that case we found that not only are the g-modes substantially modified by the rotation, but also that a new set of modes appear (the r modes) which are similar to Rossby waves in the Earth’s atmosphere and oceans.

Type
Colloquium Session VI
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 397
Copyright
Copyright © The University of Rochester 1979

References

Papaloizou, J. and Pringle, J.E. 1978. Mon.Not.R.astr.Soc., 182, 423.CrossRefGoogle Scholar
Papaloizou, J. and Pringle, J.E. 1979. Mon.Not.R.astr.Soc., in press.Google Scholar