Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-03-30
Astrophys.J. 627 (2005) 706-710
Astronomy and Astrophysics
Astrophysics
16 pages, 3 figures, Latex manuscript; accepted for publication in ApJ
Scientific paper
10.1086/430399
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 nearly 4.49, 5.55, 6.39, 7.02 and 7.85 keV), we find that a model comprising a power law (Gamma of the order of 2.2), a reflected relativistic continuum, a narrow Fe I Kalpha line from neutral material as well as a broad Fe Kalpha 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 the order of 45 degree, and an origin in a narrow region of the disk, from R_in of the order of 19 GM/c^2 to R_out of the order of 30 GM/c^2. The narrow Fe I Kalpha 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: nearly 1.4 keV for the ``double horned'' relativistic line and nearly 0.4 keV for the narrow line.
Ballo Lucia
Braito Valentina
Ceca Roberto Della
Maccacaro Tomasso
No associations
LandOfFree
The XMM-Newton view of the relativistic spectral features in AXJ0447-0627 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The XMM-Newton view of the relativistic spectral features in AXJ0447-0627, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The XMM-Newton view of the relativistic spectral features in AXJ0447-0627 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-439959