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Oscillations of rotating gas disks : p-modes, g-modes, and r-modes

Published online by Cambridge University Press:  04 August 2017

Masanori Iye
Masanori Iye*
Affiliation:
Institute of Astronomy, Cambridge CB3 0HA, U.K.

Extract

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Short-wavelength adiabatic oscillations of an infinitesimally thin, rotating and self-gravitating gas disk in dynamical equilibrium are studied. The problem is formulated in terms of the theory of oscillations of gas spheres (i.e. stars) in order to help galactic and stellar seismologists towards their mutual understanding of their rather similar subjects.

Type
PART III: Dynamics and Evolution
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 535 - 536
Copyright
Copyright © Reidel 1985 

References

Iye, M.: 1983, M.N.R.A.S. (in press).Google Scholar
Lynden-Bell, D. and Katz, J.: 1981, Proc. R. Soc. London , A378, pp.179–205.Google Scholar
Schutz, B.F. and Verdaguer, E.: 1983, M.N.R.A.S. , 202, pp.881–901.Google Scholar
Unno, W., Osaki, Y., Ando, H., and Shibahashi, H. * 1979, Nonradial Oscillations of Stars , University of Tokyo Press.Google Scholar
Verdaguer, E.: 1983, M.N.R.A.S. , 202, pp.903–925.Google Scholar