Fig. 5
Two-dimensional maps of total gas velocity fields through a cosmological AMR simulation at z = 0.6. Top left: total gas velocity (in [km s-1]); top right: turbulent velocity field captured by our new multi-scale filter; bottom left: turbulent velocity field after the removal of L ≥ 300 kpc scales; bottom right: turbulent velocity field after the removal of L ≥ 1000 kpc scales. The side of each panel is 8 Mpc h-1.
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