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The Core Helium Flash
Published online by Cambridge University Press: 12 April 2016
Abstract
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