AGN jets do not prevent the suppression of conduction by the heat buoyancy instability in simulated galaxy clusters

Open Access

Fig. 4.

Volume-weighted radial profiles of the mean plasma beta (top) and saturation coefficient f_sat (bottom) for the two choices of f_sat at three different points in time. At late times, conduction saturates at a lower value in the presence of whistler waves than in their absence.

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