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|Title:||An X-ray outflow in a luminous obscured quasar at z=1.6 in the Chandra Deep Field-South||Authors:||Vignali, C.
|Issue Date:||2014||First Page:||328||Abstract:||In the AGN-galaxy co-evolution models, AGN winds and outflows are often invoked to explain why super-massive black holes and galaxies stop growing at a certain phase of their life. They are commonly referred to as the leading actors of feedback processes, which have been recently observed in both neutral/ionized and molecular gas up to very high redshifts. Evidences for ultra-fast outflows in X-rays have been collected in the last decade of sensitive XMM-Newton, Chandra and Suzaku observations for a sizable sample of AGN, mostly at low redshift. These observations have provided important test cases for wind and feedback models. Here we present 3Ms XMM-Newton coupled to 4Ms Chandra data of an obscured luminous quasar at z=1.6 in the Chandra Deep Field South, where an outflow of velocity about 0.15c has been significantly detected.||URI:||http://hdl.handle.net/20.500.12386/12152||Bibcode ADS:||2014xru..confE.328V|
|Appears in Collections:||3.01 Contributi in Atti di convegno|
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