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Thermal Stability of Nonspherical Stars and the Solar Oblateness Problem

Published online by Cambridge University Press:  12 April 2016

Klaus J. Fricke
Klaus J. Fricke*
Affiliation:
Universitätssternwarte Göttingen, Germany

Abstract

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A brief account of the stability of distorted stars is given. From this appropriate criteria emerge, which are subsequently applied to rotational models of the sun in connection with the solar oblateness problem.

Type
Part IV / The Rotation of the Sun
Information
International Astronomical Union Colloquium , Volume 4: Stellar Rotation , 1970 , pp. 340 - 345
Copyright
Copyright © Reidel 1970

References

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