Fig. 6.
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Net mass accretion rate through concentric radial shells averaged over 3 Gyr of evolution in 500 Myr bins. The simulations without AGN show steady, smooth inflows at all radii. Simulations with AGN show, on average, lower accretion rates and more disturbed accretion patterns due to the large-scale shocks propagating outwards from the central AGN.
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