Fig. 22
Combined 3D power spectra from three clusters simulated with ENZO (Sect. 3.1), for the FLASH simulations of the sloshing cool-core in the Virgo cluster (Sect. 3.2) and of the AGN-jet in the Hydra cluster (Sect. 3.3). All spectra were normalised to have to obtain the same power at 200 kpc, while the wave numbers k are the physical ones of each simulation.
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