Grid of simulations of 10³ kicked objects, similar to Fig. 6, but showing only the objects that are in the solar neighbourhood. Again, these simulations have a fixed initial galactocentric radius, R₀ (rows: 1 kpc, 5 kpc, and 9 kpc), and a single value for v_kick (columns: 100 km s⁻¹, 400 km s⁻¹, and 700 km s⁻¹). Similarly to Fig. 6, the evolution of the galactocentric velocity (v) is shown through 2D histograms with time bins of 10 Myr and velocity bins of 30 km s⁻¹. However, since the sizes of the populations in the panels differ significantly, they are shown on different colour scales.