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The Carbon Star Luminosity Functions in the Magellanic Clouds
Published online by Cambridge University Press: 25 May 2016
Abstract
We address the question of reproducing the observed luminosity functions of carbon stars (CSLF) in both the LMC and SMC, characterized by quite different features (i.e., faint end and peak location), using a new formalism for the third dredge-up in TP-AGB models.
- Type
- Part 5. Stellar Populations and Surveys
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 372 - 373
- Copyright
- Copyright © Astronomical Society of the Pacific 1999