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The Link between Chemical Anomalies along the Red Giant Branch and the Horizontal Branch Extension in Globular Clusters

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Published 2007 November 14 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Eugenio Carretta et al 2007 ApJ 671 L125 DOI 10.1086/525021

1538-4357/671/2/L125

Abstract

We find a strong correlation between the extension of the Na-O anticorrelation observed in red giant branch (RGB) stars and the high-temperature extension of the horizontal branch (HB) blue tail of Galactic globular clusters (GCs). The longer is the O-depleted tail of the Na-O anticorrelation observed in the RGB stars, the higher the maximum temperature reached by the bluest HB stars in the GC. This result provides clear, empirical evidence of a link between the extension of the HB and the presence of star-to-star abundance variations of proton-capture elements in GC stars. We discuss the possible interpretation of this correlation.

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10.1086/525021