Helium production by low and intermediate mass stars

Physics

Scientific paper

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Abundance, Helium, Nuclear Fusion, Stellar Envelopes, Stellar Evolution, Stellar Models, Stellar Mass

Scientific paper

Processes affecting the surface helium abundance of low and intermediate mass stars are briefly reviewed. The first, second, and third dredge-ups are described, as is the envelope burning process. Prerequisites for stars to participate in these phases are mentioned, and element production during them is discussed. Synthetic models making use of these phases are briefly considered.

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