Speaker
Sebastian Heinz
(University of Madison-Wisconsin)
Description
I will discuss large scale transport in the ICM, mitigated by AGN jet feedback, and how it affects the evolution of thermal and non-thermal plasma in ICM and, in turn, the X-ray and radio properties of clusters. In particular, I will address the ability of AGN feedback to enhance conductive heat transport through a mechanism akin to the way geothermal heat pumps operate, based on a set of MHD feedback simulations of the Perseus Cluster.
Primary authors
Jennfier Stafford
(University of Wisconsin-Madison)
Prof.
Mateusz Ruszkowski
(University of Michigan-Ann Arbor)
Sebastian Heinz
(University of Madison-Wisconsin)
Dr
Torsten Ensslin
(Max-Pank Institut for Astrophysics)
Dr
Yi-Hao Chen
(University of Wisconsin-Madison)
