{ "id": "1703.04586", "version": "v1", "published": "2017-03-14T17:14:04.000Z", "updated": "2017-03-14T17:14:04.000Z", "title": "The NuSTAR view of the true Type 2 Seyfert NGC3147", "authors": [ "Stefano Bianchi", "Andrea Marinucci", "Giorgio Matt", "Riccardo Middei", "Xavier Barcons", "Loredana Bassani", "Francisco J. Carrera", "Fabio La Franca", "Francesca Panessa" ], "comment": "5 pages, 5 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.GA", "astro-ph.CO", "astro-ph.HE" ], "abstract": "We present the first NuSTAR observation of a 'true' Type 2 Seyfert galaxy. The 3-40 keV X-ray spectrum of NGC3147 is characterised by a simple power-law, with a standard {\\Gamma}~1.7 and an iron emission line, with no need for any further component up to ~40 keV. These spectral properties, together with significant variability on time-scales as short as weeks (as shown in a 2014 Swift monitoring campaign), strongly support an unobscured line-of-sight for this source. An alternative scenario in terms of a Compton-thick source is strongly disfavoured, requiring an exceptional geometrical configuration, whereas a large fraction of the solid angle to the source is filled by a highly ionised gas, whose reprocessed emission would dominate the observed luminosity. Moreover, in this scenario the implied intrinsic X-ray luminosity of the source would be much larger than the value predicted by other luminosity proxies, like the [OIII]{\\lambda}5007 emission line extinction-corrected luminosity. Therefore, we confirm with high confidence that NGC3147 is a true Type 2 Seyfert galaxy, intrinsically characterised by the absence of a BLR.", "revisions": [ { "version": "v1", "updated": "2017-03-14T17:14:04.000Z" } ], "analyses": { "keywords": [ "true type", "seyfert ngc3147", "nustar view", "seyfert galaxy", "first nustar observation" ], "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable" } } }