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Chemical Composition as a Signature of Stellar Evolution - The Barium Stars

Published online by Cambridge University Press:  19 July 2016

David L. Lambert
David L. Lambert*
Affiliation:
Department of Astronomy, The University of Texas, Austin, TX 78712 USA

Abstract

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The hypothesis that Barium stars are the product of mass transfer across a binary system is reviewed with special attention given to the chemical composition of AGB stars (the mass-losing star in the binary) and the Ba stars (the mass-gaining star).

Type
VII. Abundance Constraints on Stellar Evolution, Nucleosynthesis, and Cosmological Theories
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 563 - 576
Copyright
Copyright © Kluwer 1988 

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