{ "id": "1305.4535", "version": "v1", "published": "2013-05-20T14:11:25.000Z", "updated": "2013-05-20T14:11:25.000Z", "title": "Active Galactic Nucleus and Extended Starbursts in a Mid-stage Merger VV114", "authors": [ "D. Iono", "T. Saito", "M. S. Yun", "R. Kawabe", "D. Espada", "Y. Hagiwara", "M. Imanishi", "T. Izumi", "K. Kohno", "K. Motohara", "K. Nakanishi", "H. Sugai", "K. Tateuchi", "Y. Tamura", "J. Ueda", "Y. Yoshii" ], "comment": "5 pages, 4 figures, PASJ Letters accepted", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "High resolution (0.4 arcsec) Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 0 observations of HCO+(4-3) and HCN(4-3) toward a mid-stage infrared bright merger VV114 have revealed compact nuclear (<200 pc) and extended (3 - 4 kpc) dense gas distribution across the eastern part of the galaxy pair. We find a significant enhancement of HCN(4-3) emission in an unresolved compact and broad (290km/s) component found in the eastern nucleus of VV114, and we suggest dense gas associated with the surrounding material around an Active Galactic Nucleus (AGN), with a mass upper limit of < 4 x 10^8 Msun. The extended dense gas is distributed along a filamentary structure with resolved dense gas concentrations (230pc; 10^6 Msun) separated by a mean projected distance of 600 pc, many of which are generally consistent with the location of star formation traced in Pa alpha emission. Radiative transfer calculations suggest moderately dense (10^5 - 10^6 cm^-3) gas averaged over the entire emission region. These new ALMA observations demonstrate the strength of the dense gas tracers in identifying both the AGN and star formation activity in a galaxy merger, even in the most dust enshrouded environments in the local universe.", "revisions": [ { "version": "v1", "updated": "2013-05-20T14:11:25.000Z" } ], "analyses": { "keywords": [ "active galactic nucleus", "mid-stage merger vv114", "extended starbursts", "star formation", "atacama large millimeter/submillimeter array" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/pasj/65.3.L7", "journal": "Publications of the Astronomical Society of Japan", "year": 2013, "month": "Jun", "volume": 65 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1234202, "adsabs": "2013PASJ...65L...7I" } } }