Abstract
We present the first results of the SUMO project, aimed at studying multiple populations in globular clusters. For this purpose we obtained wide-field photometry in a large sample of clusters using both archival and proprietary U, B, V, and I data from ground-based telescopes. We have defined a new photometric index cU,B,I=(U−B)−(B−I), that we show is very effective to split multiple sequences along the red giant branch (RGB). We found a direct connection with the chemical properties of different sequences, that display different abundances of light elements.
Original language | English |
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Pages (from-to) | 4pp |
Journal | Memorie Della Societa Astronomica Italiana |
Volume | 84 |
Issue number | 71 |
Publication status | Published - 2013 |