The central engine of active galactic nuclei : proceedings of a workshop held at Xi'an Jiaotong University, Xi'an, China 16-21 October 2006

By Luis C. Ho, Jian-Min Wang. 2007

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The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS (2009, background): “The XMM-COSMOS catalog comprises 1822 point–like X-ray sources detected by XMM-Newtonover an area of∼ 2 deg2 for a total of ∼ 1.5 Ms at a fairly homogeneous depth of ∼ 50 ks (Hasinger et al. 2007, Cappelluti et al. 2009).”
THREE-DIMENSIONAL SIMULATIONS OF DYNAMICS OF ACCRETION FLOWS IRRADIATED BY A QUASAR (2007, background): “Magnetic driving is briefly discussed in §4 (see also Proga 2007).”
A Close Look at Star Formation around Active Galactic Nuclei (2007, background): “The mass-loss rate for such winds peaks at about 0.1 M yr 1 and then tails off proportionally to the K-band luminosity, leading to a cumulative mass lost of 2 ; 107 M after 1 Gyr (although most of the loss actually occurs within half of this time span).”