IC 751: a new changing-look AGN discovered by NuSTAR
arXiv:1602.00702 · doi:10.3847/0004-637X/820/1/5
Abstract
We present the results of five NuSTAR observations of the type 2 active galactic nucleus (AGN) in IC 751, three of which were performed simultaneously with XMM-Newton or Swift/XRT. We find that the nuclear X-ray source underwent a clear transition from a Compton-thick () to a Compton-thin () state on timescales of months, which makes IC 751 the first changing-look AGN discovered by NuSTAR. Changes of the line-of-sight column density at a level are also found on a time-scale of hours (). From the lack of spectral variability on timescales of ks we infer that the varying absorber is located beyond the emission-weighted average radius of the broad-line region, and could therefore be related either to the external part of the broad-line region or a clumpy molecular torus. By adopting a physical torus X-ray spectral model, we are able to disentangle the column density of the non-varying absorber () from that of the varying clouds [], and to constrain that of the material responsible for the reprocessed X-ray radiation (). We find evidence of significant intrinsic X-ray variability, with the flux varying by a factor of five on timescales of a few months in the 2-10 and 10-50 keV band.
Accepted for publication in ApJ, 11 pages, 6 figures
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