{ "id": "1208.3202", "version": "v1", "published": "2012-08-15T20:05:40.000Z", "updated": "2012-08-15T20:05:40.000Z", "title": "Chemical Analysis of a Diffuse Cloud along a Line of Sight Toward W51: Molecular Fraction and Cosmic-Ray Ionization Rate", "authors": [ "Nick Indriolo", "D. A. Neufeld", "M. Gerin", "T. R. Geballe", "J. H. Black", "K. M. Menten", "J. R. Goicoechea" ], "comment": "21 pages, 1 figure, 4 tables", "journal": "ApJ 758 (2012) 83", "categories": [ "astro-ph.GA" ], "abstract": "Absorption lines from the molecules OH+, H2O+, and H3+ have been observed in a diffuse molecular cloud along a line of sight near W51 IRS2. We present the first chemical analysis that combines the information provided by all three of these species. Together, OH+ and H2O+ are used to determine the molecular hydrogen fraction in the outskirts of the observed cloud, as well as the cosmic-ray ionization rate of atomic hydrogen. H3+ is used to infer the cosmic-ray ionization rate of H2 in the molecular interior of the cloud, which we find to be zeta_2=(4.8+-3.4)x10^-16 per second. Combining the results from all three species we find an efficiency factor---defined as the ratio of the formation rate of OH+ to the cosmic-ray ionization rate of H---of epsilon=0.07+-0.04, much lower than predicted by chemical models. This is an important step in the future use of OH+ and H2O+ on their own as tracers of the cosmic-ray ionization rate.", "revisions": [ { "version": "v1", "updated": "2012-08-15T20:05:40.000Z" } ], "analyses": { "keywords": [ "cosmic-ray ionization rate", "molecular fraction", "diffuse cloud", "diffuse molecular cloud", "molecular hydrogen fraction" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/758/2/83", "journal": "The Astrophysical Journal", "year": 2012, "month": "Oct", "volume": 758, "number": 2, "pages": 83 }, "note": { "typesetting": "TeX", "pages": 21, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1127664, "adsabs": "2012ApJ...758...83I" } } }