25 keV Observation of I13 at 171 Myr

Introduction
This is an X-ray observation of the I13 simulation at 171 Myr. We have included thermal Bremsstrahlung and inverse Compton emission from 24.5 to 25.5 keV here. To compute a realistic flux the grid was placed at 240 Mpc. The units across the bottom are 10^-23 erg s^-1 cm^-2 arcsec^-2.

At higher energies we have started to pick up significant inverse Compton emission from a within the jet material. An interesting aspect of this emission is that most of it is coming from a sheath that surrounds the cavity. This region is real mixing between ICM and AGN plasma.