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In this paper we lay out a simple set of relationships connecting thedynamics of fast plasma jets to the dynamical state of their ambient media. Theobjective is to provide a tool kit that can be used to connect the morphologiesof radio AGNs in galaxy clusters to the dynamical state of the local ICM. Theformalism is intended to apply to jets whether they are relativistic ornon-relativistic. Special attention is paid to interactions involving ICMshocks, although the results can be applied more broadly. Our formalismemphasizes the importance of the relative Mach number of the impacting ICM flowand the internal Mach number of the AGN jet in determining how the AGN outflowsevolve.

Using Collisions of AGN Outflows with ICM Shocks as Dynamical Probes