Volume 547, November 2012
|Number of page(s)||1|
|Section||Galactic structure, stellar clusters and populations|
|Published online||29 October 2012|
The Na-O anticorrelation in horizontal branch stars (Corrigendum)
II. NGC 1851⋆
INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122
2 INAF – Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
3 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
4 Astrophysics Research Institute, Liverpool John Moores University, UK
5 INAF – Osservatorio Astronomico di Teramo, via Collurania, Teramo, Italy
Key words: stars: evolution / stars: abundances / stars: Population II / globular clusters: individual: NGC 1851 / globular clusters: general / errata, addenda
The Al abundances in NGC 1851 RHB stars given in Table 3 of this paper should be corrected upward by 0.2 dex because we realized they were obtained by assuming an inconsistent, too high, solar abundance.
© ESO, 2012
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