{ "id": "1012.4802", "version": "v1", "published": "2010-12-21T21:00:00.000Z", "updated": "2010-12-21T21:00:00.000Z", "title": "Direct Evidence for an Enhancement of Helium in Giant Stars in Omega Centauri", "authors": [ "A. K. Dupree", "Jay Strader", "Graeme H. Smith" ], "comment": "ApJ in press. 29 pages, 11 figures", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "The double main sequence identified in the globular cluster Omega Centauri has been interpreted using isochrones to indicate a large variation in the abundance of helium. If true, a helium enhancement carries strong implications for the chemical and stellar evolutionary history of this cluster. However, only indirect measures currently support this conjecture. We report the discovery of a variation in the line strength of the near-infrared He I 10830 A transition in twelve similar red giants in Omega Centauri observed with PHOENIX on Gemini-S. Abundances of these stars derived from Magellan/MIKE spectra taken at Las Campanas Observatory show that the helium transition is not detected in the most metal-poor population ([Fe/H] < -1.8), yet is present in the majority of stars with [Fe/H] >= -1.8. These observations give the first direct evidence for an enhancement of helium in Omega Centauri. The appearance of helium appears better correlated with increased [Al/Fe] and [Na/Fe] abundances than as a function of [Fe/H], giving observational support to the presence of high-temperature H-burning in a prior generation of stars.", "revisions": [ { "version": "v1", "updated": "2010-12-21T21:00:00.000Z" } ], "analyses": { "keywords": [ "giant stars", "helium enhancement carries strong implications", "globular cluster omega centauri", "first direct evidence", "helium appears better" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/728/2/155", "journal": "The Astrophysical Journal", "year": 2011, "month": "Feb", "volume": 728, "number": 2, "pages": 155 }, "note": { "typesetting": "TeX", "pages": 29, "language": "en", "license": "arXiv", "status": "editable", "inspire": 882212, "adsabs": "2011ApJ...728..155D" } } }