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..195m&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

11

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.

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