Speaker
Massimo Cappi
(National Institute for Astrophysics - INAF)
Description
I will briefly review the evidence for high-velocity (mildly relativistic) and massive winds in Active Galactic Nuclei. I will then highlight some new recent results obtained in X-rays (mostly using deep XMM and Chandra observations) and at multi-frequencies for both low-z AGNs and high-z QSOs. Among other things, these studies indicate that massive, high-velocity, outflows may be more common than previously thought.
| Collaboration | INAF/IASF-Bologna |
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Primary author
Massimo Cappi
(National Institute for Astrophysics - INAF)
