Chemical abundance anomalies in globular clusters red giants

Details Chemical abundance anomalies in globular clusters red giants Chemical abundance anomalies in globular clusters red giants

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..135p&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

Most of the low-mass red giant stars that are observed in the globular clusters present abundance patterns that stellar evolution models fail to reproduce. On basis of the evolutionary scenario, which invokes an internal origin for this anomalies, we will present a rotation-induced extra-mixing process that can act on the RGB. We will then expose preliminary results concerning the effects of such a mechanism.

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