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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
Extract
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