Excitation of oscillations in roAp stars: the roles of He settling and winds

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Scientific paper

The properties of the oscillations in rapidly oscillating Ap stars strongly depend on the chemical stratification of the star. In this paper we examine the effects of a large magnetic field and various chemical transport processes (convection, He settling, turbulence and mass loss) on the chemical composition of Ap stars and on their stability. We show that the stellar evolutionary models that best reproduce the observations are those with convection suppressed, He settling and no wind. In the region of the HR diagram where most roAp stars have been found, these models predict the excitation of high frequency p modes and the damping of low frequency p modes, as observed.

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