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Studies of Non-adiabatic Effects on Radial Pulsations in the Atmospheres of Rapidly Oscillating Ap Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
A code for solving non-adiabatic radial pulsation equations with consistent treatment of radiative transfer is used to study the oscillations in the atmospheres of the rapidly oscillating Ap stars. We find that our results are consistent with the presence of an observable node in the temperature eigenfunction.
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- Part 6. Variables Close to the Main Sequence
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- Copyright © Astronomical Society of the Pacific 2000