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Rapid Pulsations in Ap Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
The rapidly oscillating Ap (roAp) stars are upper mainsequence stars that pulsate in non-radial p modes of high overtone. We present an observer’s overview of the roAp phenomenon and discuss significant developments since the last major observational reviews of Kurtz (1990a) and Matthews (1991).
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- Part 1. The Scientific Programme
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- Copyright © Astronomical Society of the Pacific 1995
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