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Pulsation Theory and Stellar Structure

Published online by Cambridge University Press:  12 April 2016

J. Christensen-Dalsgaard
J. Christensen-Dalsgaard*
Affiliation:
Institut for Fysik og Astronomi, Aarhus Universitet, DK 8000 Aarhus C, Denmark

Abstract

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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.

Type
VI. Asteroseismology: theory
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 483 - 496
Copyright
Copyright © Astronomical Society of the Pacific 1993

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