From left to right: face-on maps of the angular momentum variation ΔL, of the rotational support L_norm = L/L_circ, and of the vertical velocity dispersion σ_z for stars with different birth radii (from top to bottom: r_ini ≤ 0.4r_bar; 0.4r_bar ≤ r_ini ≤ 0.7r_bar; 0.7r_bar ≤ r_ini ≤ r_bar; r_bar ≤ r_ini ≤ 1.3r_bar; 1.3r_bar ≤ r_ini ≤ 1.6r_bar; 1.6r_bar ≤ r_ini ≤ 1.9r_bar). In this, and in all the following maps, all the quantities have been calculated over pixels whose size is 100 pc × 100 pc. The strong AM redistribution following bar formation is evident from the ΔL maps. The rotational support L_norm shown in the middle column is the ratio between the average L at a given pixel, and the AM, L_circ, that a star in circular orbit at the same location would have. In each panel, the stellar bar is aligned with the y-axis and the average initial radius is indicated by a white circle. All the plots correspond to the time t = 2.75 Gyr, as indicated. Angular momenta, and their variation, are in units of 100 km s^-1 kpc^-1; velocities in units of 100 km s^-1.