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The Effect of Coulomb Interactions on the Helium Flash
Published online by Cambridge University Press: 12 April 2016
Abstract
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Detailed evolutionary calculations show that Coulomb interactions between the charged particles of a stellar plasma reduce the core mass at which a low mass red giant undergoes the helium flash (contrary to a recent claim). This has implications for the determination of the rate of mass loss from red giants.
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- Research Article
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- Copyright © Springer-Verlag 1989
References
Renzini, A., 1977, Advanced Stages in Stellar Evolution, Ed. Iben, I., Renzini, A. and Schramm, D.N., Geneva Observatory, Switzerland.Google Scholar
Renzini, A., 1981, Effects of Mass Loss on Stellar Evolution, ed. Chiosi, C. and Stalio, R., Reidel Publishing Co., Dordrecht, Holland.Google Scholar