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Nucleosynthesis in Intermediate-Mass Stars
Published online by Cambridge University Press: 25 May 2016
Abstract
We discuss nucleosynthesis within 6 M⊙ models with Z = 0.02, 0.008 and 0.004. The emphasis is on the AGB phase of evolution, with particular reference to thermal pulses and Hot Bottom Burning. We find strong CN cycling, with substantial Al production, especially at low metallicities.
- Type
- Session X — Nucleosythesis and Evolution
- Information
- Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 449 - 458
- Copyright
- Copyright © Kluwer 2000
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