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Physical Conditions Inside White Dwarfs and Type I Supernovae

Published online by Cambridge University Press:  12 April 2016

E. Schatzman
E. Schatzman*
Affiliation:
Observatoire de NICE, France

Extract

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After the first suggestion by Schatzman (1963) that accreting white dwarfs, close to the limiting mass, might be the progenitors of type I Supernovae, the problem was not studied until Schatzman (1974) described the competition between collapse dominated by beta decay, which would lead to neutron star formation and collapse dominated by nuclear reactions leading to stellar disruption.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 72: Cataclysmic Variables and Related Objects , 1983 , pp. 149 - 153
Copyright
Copyright © Reidel 1983

References

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