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- W1569575432 abstract "A comparison of observations with models of stellar evolution is made. The following points are stressed: a) the observed mass of the ejected envelope is smaller than the predicted one, b) the observed N enrichment is larger than predicted implying that other mixing mechanisms are at play in intermediate mass stars, c) the observed He enrichment is in fair agreement with the predictions if PN originate from objects in the 1< M/M⊙< 5 range, d) in some cases the carbon abundances are considerably higher than predicted under the assumption that only matter between the hydrogen burning shell and the surface is ejected.; this is particularly the case for halo PN where also He, O, N and Ne are enriched." @default.
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- W1569575432 date "1981-01-01" @default.
- W1569575432 modified "2023-10-18" @default.
- W1569575432 title "Planetary Nebulae and Stellar Evolution" @default.
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- W1569575432 doi "https://doi.org/10.1007/978-94-009-8492-9_45" @default.
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