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AGB stars in binaries and their progeny

Published online by Cambridge University Press:  25 May 2016

A. Jorissen
A. Jorissen*
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium

Abstract

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An AGB star in a binary system is likely to pollute its companion with carbon- and s-process-rich matter. After the AGB star has faded into an unconspicuous white dwarf, the polluted companion enters the zoo of stars with chemical peculiarities. In this paper, the progeny of AGB stars in binary systems are identified among existing spectroscopic classes (Abell 35-like, binary post-AGB, WIRRing, dwarf Ba and C, subgiant CH, Ba, CH, S, yellow symbiotics) and their filiation is discussed from the properties of their eccentricity – period diagrams.

Type
Part 5. Non-Spherical Mass Loss, Binarity, Post-AGB Evolution
Information
Symposium - International Astronomical Union , Volume 191: Asymptotic Giant Branch Stars , 1999 , pp. 437 - 446
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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