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Carbon Stars in the Early-AGB Stage of Evolution
Published online by Cambridge University Press: 25 May 2016
Abstract
The assumption that faint carbon stars, as well as high-luminosity carbon stars whose effective temperatures are well above those of ordinary N-type stars in the Magellanic Clouds, are in the early asymptotic giant branch (E-AGB) evolutionary stage, is examined using population simulation techniques.
- Type
- Session X — Nucleosythesis and Evolution
- Information
- Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 463 - 467
- Copyright
- Copyright © Kluwer 2000