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The Pulsations and Evolution of AGB Stars in the Large Magellanic Cloud

Published online by Cambridge University Press:  25 May 2016

Z. G. Gong  and
Y. Li
Z. G. Gong
Affiliation:
Yunnan Observatory, Kunming, P. R. China
Y. Li
Affiliation:
Yunnan Observatory, Kunming, P. R. China

Abstract

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The evolutionary status and pulsational characteristics of AGB stars in the LMC have been studied. It is found that only those stars with a small mixing-length ratio can fit the observed period-luminosity relation. Strong non-adiabatic effects were found in the outer envelope and must be taken into account in future work.

Type
Session IV — Variability
Information
Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 199 - 204
Copyright
Copyright © Kluwer 2000 

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