{ "id": "1305.5975", "version": "v2", "published": "2013-05-26T00:11:03.000Z", "updated": "2013-09-23T19:08:24.000Z", "title": "Super-Massive Stars as a Source of Abundance Anomalies of Proton-Capture Elements in Globular Clusters", "authors": [ "Pavel A. Denissenkov", "F. D. A. Hartwick" ], "comment": "5 pages, 3 figures, accepted for publication in MNRAS Letters", "categories": [ "astro-ph.SR" ], "abstract": "We propose that the abundance anomalies of proton-capture elements in globular clusters, such as the C-N, Na-O, Mg-Al and Na-F anti-correlations, were produced by super-massive stars with M ~ 10,000 Msun. Such stars could form in the runaway collisions of massive stars that sank to the cluster center as a result of dynamical friction, or via the direct monolithic collapse of the low-metallicity gas cloud from which the cluster formed. To explain the observed abundance anomalies, we assume that the super-massive stars had lost significant parts of their initial masses when only a small mass fraction of hydrogen, Delta X ~ 0.15, was transformed into helium. We speculate that the required mass loss might be caused by the super-Eddington radiation continuum-driven stellar wind or by the diffusive mode of the Jeans instability.", "revisions": [ { "version": "v2", "updated": "2013-09-23T19:08:24.000Z" } ], "analyses": { "keywords": [ "abundance anomalies", "super-massive stars", "proton-capture elements", "globular clusters", "super-eddington radiation continuum-driven stellar wind" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnrasl/slt133", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2014, "month": "Jan", "volume": 437, "number": 1 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1235491, "adsabs": "2014MNRAS.437L..21D" } } }