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The Chemical Composition of Asymptotic Giant Branch Stars

Published online by Cambridge University Press:  12 April 2016

David L. Lambert
David L. Lambert*
Affiliation:
Department of Astronomy, University of Texas, Austin, Texas

Abstract

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Low resolution spectroscopic and photometric studies of Magellanic Cloud AGB stars have shown that the M → S → C sequence is the result of the third dredge-up of 12C and s-process elements in AGB stars of low mass. In this paper, data on the chemical compositions of normal Galactic M → S → C stars are reviewed and shown to be broadly consistent with expectations for the third dredge-up on the AGB.

Type
2. Model Photospheres and Chemical Compositions
Information
International Astronomical Union Colloquium , Volume 106: Evolution of Peculiar Red Giant Stars , 1989 , pp. 101 - 130
Copyright
Copyright © Cambridge University Press 1989

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