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20. Gravitational Sorting and Overstability in White Dwarfs

Published online by Cambridge University Press:  14 August 2015

A. Baglin
A. Baglin*
Affiliation:
Observatoire de Nice, Nice, France

Extract

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Zones with μ gradient in stars have been discussed extensively in recent years in relation with the so-called ‘semi-convective zone’ which forms in massive stars when the convective core shrinks.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 42: White Dwarfs , 1971 , pp. 136 - 144
Copyright
Copyright © Reidel 1971 

References

Auré, J. L.: 1970, Astron. Astrophys., in press.Google Scholar
Chapman, S. and Cowling, T. G.: 1960, The Mathematical Theory of Non-Uniform Gases, Reprinted Dover, New York.Google Scholar
Gabriel, M.: 1969, Astron. Astrophys. 1, 321.Google Scholar
Kato, S.: 1966, PASJ 18, 374.Google Scholar
Ledoux, P. and Walraven, T.: 1958, Handbuch der Physik 51, Springer-Verlag.Google Scholar
Schatzman, E.: 1958, White Dwarfs, North-Holland Publ. Co., Amsterdam.Google Scholar
Vauclair, G.: 1970, to be published.Google Scholar