{ "id": "1506.03333", "version": "v1", "published": "2015-06-10T14:47:27.000Z", "updated": "2015-06-10T14:47:27.000Z", "title": "First Detection of HCO$^+$ Absorption in the Magellanic System", "authors": [ "Claire E. Murray", "Snežana Stanimirović", "N. M. McClure-Griffiths", "M. E. Putman", "H. S. Liszt", "Tony Wong", "P. Richter", "J. R. Dawson", "John M. Dickey", "Robert R. Lindner", "Brian L. Babler", "J. R. Allison" ], "comment": "Accepted for publication in ApJ. 6 pages, 2 figures, 2 tables", "categories": [ "astro-ph.GA" ], "abstract": "We present the first detection of HCO$^+$ absorption in the Magellanic System. Using the Australia Telescope Compact Array (ATCA), we observed 9 extragalactic radio continuum sources behind the Magellanic System and detected HCO$^+$ absorption towards one source located behind the leading edge of the Magellanic Bridge. The detection is located at LSR velocity of $v=214.0 \\pm 0.4\\rm\\,km\\,s^{-1}$, with a full width at half maximum of $\\Delta v=4.5\\pm 1.0\\rm\\,km\\,s^{-1}$ and optical depth of $\\tau(\\rm HCO^+)=0.10\\pm 0.02$. Although there is abundant neutral hydrogen (HI) surrounding the sightline in position-velocity space, at the exact location of the absorber the HI column density is low, $<10^{20}\\rm\\,cm^{-2}$, and there is little evidence for dust or CO emission from Planck observations. While the origin and survival of molecules in such a diffuse environment remains unclear, dynamical events such as HI flows and cloud collisions in this interacting system likely play an important role.", "revisions": [ { "version": "v1", "updated": "2015-06-10T14:47:27.000Z" } ], "analyses": { "keywords": [ "magellanic system", "first detection", "absorption", "australia telescope compact array", "extragalactic radio continuum sources" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }