The XMM- Newton observation of the optically Type 1 AGN AXJ0447-0627 ( z = 0.214 ) unambiguously reveals a complex , bright and prominent set of lines in the 4 - 8 \ > keV rest frame energy range .
Although , from a phenomenological point of view , the observed properties can be described by a simple power law model plus 5 narrow Gaussian lines ( at rest frame energies of \sim 4.49 , \sim 5.55 , \sim 6.39 , \sim 7.02 and \sim 7.85 \ > keV ) , we find that a model comprising a power law ( \Gamma \sim 2.2 ) , a reflected relativistic continuum , a narrow Fe I K \alpha line from neutral material as well as a broad Fe K \alpha relativistic line from a ionized accretion disk represents a good physical description of the data .
The “ double horned ” profile of the relativistic line implies an inclination of the accretion disk of \sim 45 ^ { \circ } , and an origin in a narrow region of the disk , from R _ { \mbox { \scriptsize in } } \sim 19 \ > GM / c ^ { 2 } to R _ { \mbox { \scriptsize out } } \sim 30 \ > GM / c ^ { 2 } .
The narrow Fe I K \alpha line from neutral material is probably produced far from the central black hole , most likely in the putative molecular torus .
Although some of these properties have been already found in other Type 1 AGN and discussed in the literature , at odd with the objects reported so far we measure high equivalent widths ( EWs ) of the observed lines : \sim 1.4 \ > keV for the “ double horned ” relativistic line and \sim 0.4 \ > keV for the narrow line .