Red giant stars - Comparison of observations and theory

Details Red giant stars - Comparison of observations and theory Red giant stars - Comparison of observations and theory

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..207m&link_type=abstract

IN: Structure and evolution of the Magellanic Clouds; Proceedings of the Symposium, Tuebingen, West Germany, September 5-8, 1983

Physics

Magellanic Clouds, Red Giant Stars, Stellar Evolution, Stellar Mass Ejection, Asymptotic Giant Branch Stars, Carbon Stars, Nuclear Fusion, Stellar Luminosity

Scientific paper

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.

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