{ "id": "1209.6420", "version": "v1", "published": "2012-09-28T04:14:20.000Z", "updated": "2012-09-28T04:14:20.000Z", "title": "Detection of Interstellar C_2 and C_3 in the Small Magellanic Cloud", "authors": [ "Daniel E. Welty", "J. Christopher Howk", "Nicolas Lehner", "John H. Black" ], "comment": "accepted to MNRAS; 10 pages, 6 figures", "categories": [ "astro-ph.GA" ], "abstract": "We report the detection of absorption from interstellar C_2 and C_3 toward the moderately reddened star Sk 143, located in the near 'wing' region of the SMC, in optical spectra obtained with the ESO VLT/UVES. These detections of C_2 (rotational levels J=0-8) and C_3 (J=0-12) absorption in the SMC are the first beyond our Galaxy. The total abundances of C_2 and C_3 (relative to H_2) are similar to those found in diffuse Galactic molecular clouds -- as previously found for CH and CN -- despite the significantly lower average metallicity of the SMC. Analysis of the rotational excitation of C_2 yields an estimated kinetic temperature T_k ~ 25 K and a moderately high total hydrogen density n_H ~ 870 cm^-3 -- compared to the T_01 ~ 45 K and n_H ~ 85-300 cm^-3 obtained from H_2. The populations of the lower rotational levels of C_3 are consistent with an excitation temperature of about 34 K.", "revisions": [ { "version": "v1", "updated": "2012-09-28T04:14:20.000Z" } ], "analyses": { "keywords": [ "small magellanic cloud", "interstellar", "moderately high total hydrogen density", "diffuse galactic molecular clouds", "lower rotational levels" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnras/sts093", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2013, "month": "Jan", "volume": 428, "number": 2, "pages": 1107 }, "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1188643, "adsabs": "2013MNRAS.428.1107W" } } }