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The Core Helium Flash
Published online by Cambridge University Press: 12 April 2016
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
Deupree, R. G. and CoLe, P. W.: 1980, in Fischel, D., Lesh, J., and Sparks, W. M. (eds.), Current Problems in Stellar Pulsation Instabilities, NASA Technical Memorandum 80625, p. 113.Google Scholar
Wickett, A. J.: 1977, in Spiegel, E. A. and Zahn, J. P. (eds.), Problems of Stellar Convection, p. 284.CrossRefGoogle Scholar