{ "id": "1603.02827", "version": "v1", "published": "2016-03-09T09:50:16.000Z", "updated": "2016-03-09T09:50:16.000Z", "title": "Multiple stellar populations in the globular cluster M3 (NGC 5272): a Strömgren perspective", "authors": [ "Davide Massari", "Emilio Lapenna", "Angela Bragaglia", "Emanuele Dalessandro", "Rodrigo Contreras Ramos", "Pia Amigo" ], "comment": "11 pages, 9 figures, 2 tables. Accepted for publication in MNRAS", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "We present Str\\\"omgren photometry of the Galactic Globular Cluster M3 to study its multiple generations phenomenon. The use of different colour-magnitude diagrams and especially of the notoriously efficient c_y index allowed us to detect a double Red Giant Branch in the cluster CMD. After decontamination from fore- and background sources, the two sequences turned out to be equally populated. The two components also show a bimodal radial distribution well corresponding to that predicted by numerical simulations for clusters living in an intermediate dynamical evolutive state and with a population with modified chemical composition that was born more centrally concentrated than the primordial. The analysis of high-resolution spectra quantitatively demonstrates that the two detected sequences correspond to the first (Na-poor) generation and the second (Na-rich) generation, thus confirming the importance of synergy between photometry and spectroscopy.", "revisions": [ { "version": "v1", "updated": "2016-03-09T09:50:16.000Z" } ], "analyses": { "keywords": [ "multiple stellar populations", "strömgren perspective", "galactic globular cluster m3", "multiple generations phenomenon", "high-resolution spectra quantitatively demonstrates" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016arXiv160302827M" } } }