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Norman R. Simon Papers
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Document Type
Article
Date of this Version
3-23-1972
Citation
Astron. & Astrophys. 21, 51-55 (1972).
Abstract
An iterative technique is used to calculate radial adiabatic pulsational amplitudes up to second order in a very massive main-sequence star. The second order terms are displayed, and discussed in detail. A possible connection between the qualitative structure of these terms and the absence of observed massive main-sequence pulsators is suggested. Finally, we discuss the resonance properties of the present model and consider their effect on the iterative calculation.
COinS
Comments
Copyright 1972 European Southern Observatory