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Pulsation Theory and Stellar Structure
Published online by Cambridge University Press: 12 April 2016
Abstract
Observed periods of pulsating stars provide information about the properties of the stars. As examples I here consider double-mode pulsators, solar-like oscillations and δ Scuti stars. The ongoing expansion in the observational efforts in this area may be expected to lead to increasingly detailed tests of stellar evolution theory.
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- VI. Asteroseismology: theory
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- Copyright © Astronomical Society of the Pacific 1993
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