{ "id": "1711.08183", "version": "v1", "published": "2017-11-22T09:12:51.000Z", "updated": "2017-11-22T09:12:51.000Z", "title": "12C/13C isotopic ratios in red-giant stars of the open cluster NGC 6791", "authors": [ "László Szigeti", "Szabolcs Mészáros", "Verne V. Smith", "Katia Cunha", "Nadège Lagarde", "Corinne Charbonnel", "Matthew Shetrone", "Marc Pinsonneault", "Carlos Allende Prieto", "J. G. Fernández-Trincado", "József Kovács", "Sandro Villanova" ], "comment": "Accepted for publication in MNRAS, 9 pages, 4 figures, 2 tables", "categories": [ "astro-ph.SR" ], "abstract": "Carbon isotope ratios, along with carbon and nitrogen abundances, are derived in a sample of 11 red-giant members of one of the most metal-rich clusters in the Milky Way, NGC 6791. The selected red-giants have a mean metallicity and standard deviation of [Fe/H]=+0.39+-0.06 (Cunha et al. 2015). We used high resolution H-band spectra obtained by the SDSS-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE). The advantage of using high-resolution spectra in the H-band is that lines of CO are well represented and their line profiles are sensitive to the variation of 12C/13C. Values of the 12C/13C ratio were obtained from a spectrum synthesis analysis. The derived 12C/13C ratios varied between 6.3 and 10.6 in NGC 6791, in agreement with the final isotopic ratios from thermohaline-induced mixing models. The ratios derived here are combined with those obtained for more metal poor red-giants from the literature to examine the correlation between 12C/13C, mass, metallicity and evolutionary status.", "revisions": [ { "version": "v1", "updated": "2017-11-22T09:12:51.000Z" } ], "analyses": { "keywords": [ "open cluster ngc", "12c/13c isotopic ratios", "red-giant stars", "point observatory galactic evolution experiment", "apache point observatory galactic evolution" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }