{ "id": "1311.4988", "version": "v1", "published": "2013-11-20T09:31:48.000Z", "updated": "2013-11-20T09:31:48.000Z", "title": "TERZAN 5: the remnant of a pristine fragment of the Galactic Bulge?", "authors": [ "Barbara Lanzoni", "the Cosmic-Lab Team" ], "comment": "Proceeding of the EWASS 2013 Conference, S5: \"Local group, local cosmology\" (8-9 July 2013, Turku, Finland), Mem. S.A.It, M. Monelli and S. Salvadori Eds", "categories": [ "astro-ph.GA" ], "abstract": "Terzan 5 is a stellar system in the Galactic bulge commonly catalogued as a globular cluster. Through dedicated NIR photometry and spectroscopy we have discovered that it harbors two main stellar populations defining two distinct red clumps (RCs) in the colour-magnitude diagram, and displaying different iron content: [Fe/H] = -0.2 and [Fe/H]=+0.3 for the faint and the bright red clumps, respectively. In addition, a third minor population with significantly lower metallicity ([Fe/H]=-0.79) has been recently detected, thus enlarging the metallicity range covered by Terzan 5 to Delta[Fe/H] ~ 1 dex. This evidence demonstrates that, similarly to omega Centauri in the Galactic halo, Terzan 5 is not a genuine globular cluster, but a stellar system that experienced a much more complex star formation and chemical enrichment history. Moreover the striking chemical similarity with the bulge stars suggests that Terzan 5 could be the relic of one of the massive clumps that contributed through strong dynamical interactions with other similar sub-structures) to the formation of the Galactic bulge.", "revisions": [ { "version": "v1", "updated": "2013-11-20T09:31:48.000Z" } ], "analyses": { "keywords": [ "galactic bulge", "pristine fragment", "stellar system", "third minor population", "genuine globular cluster" ], "tags": [ "conference paper" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014MmSAI..85..536L" } } }