{ "id": "1806.04922", "version": "v1", "published": "2018-06-13T10:04:20.000Z", "updated": "2018-06-13T10:04:20.000Z", "title": "Galactic HCO+ Absorption toward Compact Extragalactic Radio Sources", "authors": [ "Geumsook Park", "Bon-Chul Koo", "Kee-Tae Kim", "Do-Young Byun", "Carl E. Heiles" ], "comment": "10 pages, 3 figures; accepted in Astrophysics and Space Science (ASTR-D-18-00258R1)", "categories": [ "astro-ph.GA" ], "abstract": "As part of the search for the \"dark molecular gas (DMG),\" we report on the results of HCO$^+$ J = 1-0 absorption observations toward nine bright extragalactic millimeter wave continuum sources. The extragalactic sources are at high Galactic latitudes (|b| > 10$\\deg$) and seen at small extinction (E(B-V) $\\lesssim$ 0.1 mag). We have detected the HCO$^+$ absorption lines toward two sources, B0838+133 and B2251+158. The absorption toward B2251+158 was previously reported, while the absorption toward B0838+133 is a new detection. We derive hydrogen column densities or their upper limits toward the nine sources from our observations and compare them to those expected from CO line emission and far-infrared dust continuum emission. Toward the seven sources with no HCO$^+$ detection, CO emission has not been detected, either. Thus the sight lines are likely to be filled with almost pure atomic gas. Toward the two sources with HCO$^+$ detection, CO emission has been also detected. Comparison of the H$_2$ column densities from HCO$^+$ absorption and CO emission suggests a non-negligible amount of DMG toward B0838+133.", "revisions": [ { "version": "v1", "updated": "2018-06-13T10:04:20.000Z" } ], "analyses": { "keywords": [ "compact extragalactic radio sources", "absorption", "bright extragalactic millimeter wave continuum", "extragalactic millimeter wave continuum sources", "column densities" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }