Halo cloud radial velocity statistics given as a probability distribution. The colored graphs show the distributions for the three simulations individually as well as their average in black. The red line shows the result from Ramesh et al. (2023), who conducted a similar analysis based on 132 Milky Way-like halos from the TNG50 simulation. For a description of their galaxy sample we refer to Sect. 4.3. The hatched area highlights the low-velocity region with |v_LSR| ≤ 100 km s⁻¹. The histogram is binned into bins with a width of 50 km s⁻¹.