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A model for cosmological simulations of galaxy formation physics

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Figure

Figure 1. Influence of the AGN radiation field (“electro-magnetic feedback”) on the net cooling rate for gases of different metallicities, in the rangelog[Z/Z⊙]=−2.0, −1.0, 0.0, 1.0 (lowest to highest curve)
Table 1. Fiducial model parameters. We assume purely energy-driven, non-local winds for stellar feedback
Figure 2. Gas density (left panel), gas temperature (middle panel) and gas metallicity (right panel) projections of the L25n512 simulation
Figure 3. Gas density (left panel), gas temperature (middle panel) and gas metallicity (right panel) projections of the L25n256 simulation (top panels) and“no feedback” simulation (bottom panels) at z = 0
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