Piazzale Aldo Moro

Jul 5, 2024 | academic.oup.com | Tor Vergata |Piazzale Aldo Moro |Reggio Emilia

Powerful supermassive black hole (SMBH) winds in the form of ultra-fast outflows (UFOs) are detected in the X-ray spectra of several active galactic nuclei (AGN) seemingly independently of their radio classification between radio quiet (RQ) and radio loud (RL). In this work we explore the physical parameters of SMBH winds through a uniform analysis of a sample of X-ray bright RQ and RL AGN.