{ "id": "0710.5503", "version": "v2", "published": "2007-10-29T19:15:52.000Z", "updated": "2008-01-10T20:04:08.000Z", "title": "High-ionization mid-infrared lines as black hole mass and bolometric luminosity indicators in active galactic nuclei", "authors": [ "K. M. Dasyra", "L. C. Ho", "L. Armus", "P. Ogle", "G. Helou", "B. M. Peterson", "D. Lutz", "H. Netzer", "E. Sturm" ], "comment": "accepted for publication in ApJL", "doi": "10.1086/528843", "categories": [ "astro-ph" ], "abstract": "We present relations of the black hole mass and the optical luminosity with the velocity dispersion and the luminosity of the [Ne V] and the [O IV] high-ionization lines in the mid-infrared (MIR) for 28 reverberation-mapped active galactic nuclei. We used high-resolution Spitzer Infrared Spectrograph and Infrared Space Observatory Short Wavelength Spectrometer data to fit the profiles of these MIR emission lines that originate from the narrow-line region of the nucleus. We find that the lines are often resolved and that the velocity dispersion of [Ne V] and [O IV] follows a relation similar to that between the black hole mass and the bulge stellar velocity dispersion found for local galaxies. The luminosity of the [Ne V] and the [O IV] lines in these sources is correlated with that of the optical 5100A continuum and with the black hole mass. Our results provide a means to derive black hole properties in various types of active galactic nuclei, including highly obscured systems.", "revisions": [ { "version": "v2", "updated": "2008-01-10T20:04:08.000Z" } ], "analyses": { "keywords": [ "black hole mass", "active galactic nuclei", "bolometric luminosity indicators", "high-ionization mid-infrared lines", "short wavelength spectrometer data" ], "tags": [ "journal article" ], "publication": { "journal": "The Astrophysical Journal", "year": 2008, "month": "Feb", "volume": 674, "number": 1 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 765924, "adsabs": "2008ApJ...674L...9D" } } }