The link between chemical anomalies along the red giant branch and the horizontal branch extension in globular clusters

被引:39
作者
Carretta, Eugenio [1 ]
Recio-Blanco, Alejandra [2 ]
Gratton, Raffaele G. [3 ]
Piotto, Giampaolo [4 ]
Bragaglia, Angela [1 ]
机构
[1] Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy
[2] Observ Cote Azur, CNRS, UMR 6202, Dept Cassiopee, F-06304 Nice 4, France
[3] Osservatorio Padova, INAF, I-35122 Padua, Italy
[4] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
关键词
globular clusters : general; stars : abundances; stars : evolution;
D O I
10.1086/525021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:L125 / L128
页数:4
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