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Fig. 2.


Top panel: time evolution of cluster properties including stellar mass Mstar, SMBH mass MSMBH and gas mass Mgas. Middle panel: AGN luminosity, X-ray luminosity of hot gas within 50 kpc of the cluster centre, and the dense mass again for comparison. Bottom panel: SFR, as well as the dense gas mass again for comparison, for both the fiducial simulation and for a companion simulation without metal cooling for gas with T >  104 K (see text for details). Dense gas is defined to be gas with a temperature at or below Tdense = 106 K, hot, diffuse gas with a temperature above that. White and grey background colours show the heating and cooling dominated regimes of the fiducial simulation.

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