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Seismology of the ZZ Ceti Stars

Published online by Cambridge University Press:  08 February 2017

J. Christopher Clemens
J. Christopher Clemens*
Affiliation:
Palomar Observatory, 105-24, California Institute of Technology, Pasadena, CA 91125

Abstract

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The pulsations of white dwarf stars are potentially a rich source of information about white dwarf structural properties. Extracting and applying this information to improve our knowledge of white dwarf interiors requires measuring individual eigenperiods in a complex power spectrum, and identifying the character of the eigenmodes they represent. This review will summarize observational progress in these areas for the ZZ Ceti pulsators.

Type
V. Asteroseismology I
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 253 - 260
Copyright
Copyright © Kluwer 1998 

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