Orlowski-Scherer, John; Haridas, Saianeesh K.; Di Mascolo, Luca; Sarmiento, Karen Perez; Romero, Charles E.; Dicker, Simon; Mroczkowski, Tony; Bhandarkar, Tanay; Churazov, Eugene; Clarke, Tracy E.; Devlin, Mark; Gaspari, Massimo; Lowe, Ian; Mason, Brian; Sarazin, Craig L.; Sievers, Jonathon; Sunyaev, Rashid
(2022)
Context. Mechanical feedback from active galactic nuclei is thought to be the dominant feedback mechanism quenching cooling flows and star formation in galaxy cluster cores. It, in particular, manifests itself by creating ...