{ "id": "1707.02310", "version": "v1", "published": "1970-01-01T00:00:00.000Z", "updated": "2017-07-07T18:00:35.000Z", "title": "Carbon-enhanced metal-poor stars in the SDSS-APOGEE database", "authors": [ "Collin L. Kielty", "Kim A. Venn", "Nicholas B. Loewen", "Matthew D. Shetrone", "Vinicius M. Placco", "Farbod Jahandar", "Szabolcs Mészáros", "Sarah L. Martell" ], "comment": "20 pages, 9 tables, 9 figures: Accepted for publication in MNRAS", "doi": "10.1093/mnras/stx1594", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "We identify six new CEMP stars ([C/Fe]>+0.7 and [Fe/H]< -1.8) and another seven likely candidates within the APOGEE database following Data Release 12. These stars have chemical compositions typical of metal-poor halo stars, e.g., mean [$\\alpha$/Fe] = +0.24$\\pm$0.24, based on the ASPCAP pipeline results. A lack of heavy element spectral lines impedes further sub-classification of these CEMP stars, however, based on radial velocity scatter, we predict most are not CEMP-s stars which are typically found in binary systems. Only one object, 2M15312547+4220551, may be in a binary since it exhibits a scatter in its radial velocity of 1.7 $\\pm$0.6 km s$^{-1}$ based on three visits over a 25.98 day baseline. Optical observations are now necessary to confirm the stellar parameters and low metallicities of these stars, to determine the heavy-element abundance ratios and improve the precision in the derived abundances, and to examine their CEMP sub-classifications.", "revisions": [ { "version": "v0", "updated": "1970-01-01T00:00:00.000Z", "title": "", "abstract": "", "comment": null, "journal": null, "doi": null, "authors": [] }, { "version": "v1", "updated": "2017-07-07T18:00:35.000Z" } ], "analyses": { "keywords": [ "carbon-enhanced metal-poor stars", "sdss-apogee database", "heavy element spectral lines impedes", "cemp stars", "aspcap pipeline results" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 20, "language": "en", "license": "arXiv", "status": "editable" } } }