G. Beccari, M. Bellazzini, C. Lardo, A. Bragaglia, E. Carretta, E. Dalessandro, A. Mucciarelli, E. Pancino
We present accurate wide-field uVI photometry of the remote and massive Galactic globular cluster NGC 2419, aimed at searching for the u-V color spread along the Red Giant Branch (RGB) that is generally interpreted as the photometric signature of the presence of multiple populations in globular clusters. Focusing on the RGB stars in the magnitude range 19.80.0 lie preferentially on the blue side.
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http://arxiv.org/abs/1302.4375
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