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The Chemical Composition and Orbital Parameters of Barium Stars
Published online by Cambridge University Press: 25 May 2016
Abstract
The observational relation between s-process abundance anomalies and orbital periods for barium stars is discussed and compared with mass-transfer simulations. Recent detailed abundance analyses of a large sample of single-lined long-period binaries provide evidence that all giants with white dwarf companions are likely to have abundance anomalies.
- Type
- Session VI — Binarity
- Information
- Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 277 - 284
- Copyright
- Copyright © Kluwer 2000
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