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g Modes in F Stars – A Non-adiabatic Investigation of the Stability of g Modes in ϒ Doradus Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
We investigate a sequence of 1.5 M⊙ models for g-mode instabilities. For the computation of the nonradial, non-adiabatic oscillations we make use of the Riccati method introduced by Glatzel & Gautschy (1992) to integrate the pulsation equations as given by Unno et al. (1989).
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- Part 6. Variables Close to the Main Sequence
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- Copyright © Astronomical Society of the Pacific 2000
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