Go with the flow: The self-similar and non-linear behaviour of large-scale in- and outflows and the impact of accretion shocks from galaxies to galaxy clusters

Open Access

Fig. 6.

Redshift evolution of inflow, outflow, and net flow (inflow − outflow) at 1.2r_vir (top row) and at 2.0r_vir (bottom row). The bin masses (x-axis) are identical to the ones used in Fig. 3. The colours indicate the redshift of the curve.

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