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Red Giant Stars: Comparison of Observations and Theory

Published online by Cambridge University Press:  04 August 2017

Jeremy Mould
Jeremy Mould*
Affiliation:
Palomar Observatory, California Institute of Technology

Abstract

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Recent observations in both the field and the clusters of the Magellanic Clouds suggest a higher mass loss rate during or at the end of the asymptotic giant branch phase than previously supposed. Recent theoretical investigations offer an explanation for the frequency of carbon stars in the Clouds, but a rich parameter space remains to be explored, before detailed agreement can be expected.

Type
Stellar Populations
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 195 - 206
Copyright
Copyright © Reidel 1984 

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