Mixing along the red giant branch

Details Mixing along the red giant branch Mixing along the red giant branch

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..154w&link_type=abstract

In: Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 J

Astronomy and Astrophysics

Astronomy

Red Giant Branch, Low-Mass Stars

Scientific paper

Abundance analysis in globular clusters are precious clues to the chemical history of these systems. While some of so-called abundance anomalies exhibited by GC RGB stars are the chemical fingerprints of previous stellar populations some of them result from nucleosynthesis and mixing in the stars we do observe now. In this talk we concentrate on this latter aspect and we discuss in particular the effects of rotation-induced mixing.

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