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The Core Helium Flash

Published online by Cambridge University Press:  12 April 2016

Peter W. Cole  and
Robert G. Deupree
Peter W. Cole
Affiliation:
Department of Astronomy, Boston University
Robert G. Deupree
Affiliation:
Department of Astronomy, Boston University and Los Alamos Scientific Laboratory

Abstract

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The role of convection in the core helium flash is simulated by two-dimensional eddies interacting with the thermonuclear runaway. These eddies are followed by the explicit solution of the 2D conservation laws with a 2D finite difference hydrodynamics code. Thus, no phenomenological theory of convection such as the local mixing length theory is required.

Type
VII. RR Lyrae and BL Herculis Variables
Information
International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 491 - 493
Copyright
Copyright © Reidel 1980

References

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