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Carbon Stars and Nucleosynthesis in Galaxies

Published online by Cambridge University Press:  25 May 2016

Bengt Gustafsson  and
Nils Ryde
Bengt Gustafsson
Affiliation:
Uppsala Astronomical Observatory, Uppsala, Sweden
Nils Ryde
Affiliation:
Uppsala Astronomical Observatory, Uppsala, Sweden

Abstract

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The role of carbon stars in the build-up of chemical elements in galaxies is discussed on the basis of stellar evolution calculations and estimated stellar yields, abundance analyses of AGB stars, galactic-evolution models and abundance trends among solar-type disk stars. We conclude that the AGB stars in general, and carbon stars in particular, probably are main contributors of s-elements, that their contributions of flourine and carbon are quite significant, and that possibly their contributions of lithium, 13C and 22Ne are of some importance. Also contributions of N, Na and Al are discussed. The major uncertainties that characterize almost any statement concerning these issues are underlined.

Type
Session XI — Galactic Chemical Evolution
Information
Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 481 - 496
Copyright
Copyright © Kluwer 2000 

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