High Velocity Outflows in Narrow Absorption Line Quasars

The current paradigm for the AGN phenomenon is a central engine that consists of an inflow of material accreting in the form of a disk onto a supermassive black hole. Observations in the UV and optical find high velocity ionized material outflowing from the black hole. We present results from Suzaku and XMM-Newton observations of a sample of intrinsic NAL quasars with high velocity outflows. Our derived values of the intrinsic column densities of the X-ray absorbers are consistent with an outflow scenario in which NAL quasars are viewed at smaller inclination angles than BAL quasars. We find that the distributions of αOX and ∆αOX of the NAL quasars of our sample differ significantly from those of BAL quasars and SDSS radio-quiet Preprint submitted to New Astronomy Reviews July 20, 2009 quasars. The NAL quasars are not significantly absorbed in the X-ray band and the positive values of ∆αOX suggest absorption in the UV band. The positive values of ∆αOX of the intrinsic NAL quasars can be explained in a geometric scenario where our lines of sight towards the compact X-ray hot coronae of NAL quasars do not traverse the absorbing wind whereas lines of sight towards their UV emitting accretion disks do intercept the outflowing absorbers.