Probing Broad Absorption Line Quasar Outflows: X-ray Insights
  Energetic outflows appear to occur in conjunction with active mass accretion onto supermassive black holes. These outflows are most readily observed in the approximately 10% of quasars with broad absorption lines, where the observer's line of sight passes through the wind. Until fairly recently, the paucity of X-ray data from these objects was notable, but now sensitive hard-band missions such as Chandra and XMM-Newton are routinely detecting broad absorption line quasars. The X-ray regime offers qualitatively new information for the understanding of these objects, and these new results must be taken into account in theoretical modeling of quasar winds. 
S.C. Gallagher (MIT), W.N. Brandt, G. Chartas, G.P. Garmire (Penn   State), and R.M. Sambruna (George Mason)