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How to drive roAp stars

Alfred Gautschy·Hideyuki Saio·Housi Harzenmoser
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Abstract

Rapidly oscillating Ap stars consitute a unique class of pulsators to study nonradial oscillations under some - even for stars - unusual physical conditions. These stars are chemically peculiar, they have strong magnetic fields, and they often pulsate in several high-order acoustic modes simultaneously. We discuss here an excitation mechanism for short-period oscillation modes based on the classical kappa mechanism. We particularly stress the conditions that must be fulfilled for successful driving. Specifically, we discuss the roles of chemical peculiarity and strong magnetic field on the oscillation modes and what separates these pulsators from delta Scuti and Am-type stars.

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Alfred Gautschy, Hideyuki Saio, Housi Harzenmoser. 1998-06-22. How to drive roAp stars. https://doi.org/10.1046/j.1365-8711.1998.01960.x

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