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Models of AGB Stars Envelopes and Atmospheres
Published online by Cambridge University Press: 12 April 2016
Extract
The possible existence of a hot CN-cycle at the bottom of the AGB convective envelopes (“hot-bottom burning” or HBB) encounters some revealing difficulties with observations (e.g. Reid and mould, 1985). On the other hand, existing models disagree with each other about it.
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- 3. Evolution of Peculiar Red Giant Stars
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- Copyright © Cambridge University Press 1989