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Binarity and Abundance Anomalies in Stars

Published online by Cambridge University Press:  19 July 2016

A. V. Tutukov
A. V. Tutukov*
Affiliation:
The Astronomical Council of the Academy of Sciences of the USSR Pyatnitskaya str. 48, Moscow 109017, U.S.S.R.

Abstract

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About one half of all stars are close binaries whose components can efficiently interact during their evolution. The interaction of the components significantly influences the evolution and changes the chemical composition of their atmospheres. This review is devoted to the discussion of the binarity role in the creation of stars with an anomalous chemical composition of their envelopes: WR, OBN, OBC, RCrB, Ba, sdBO, Am, Fm, Ap, Bp, helium stars, CO stars, Na giants.

Type
Horizontal Branch Stars and Binaries
Information
Symposium - International Astronomical Union , Volume 145: Evolution of Stars: The Photospheric Abundance Connection , 1991 , pp. 351 - 362
Copyright
Copyright © Kluwer 1991 

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