Ratio between the standard deviations of V_i and V_circ (ΔV_i/ΔV_circ) at z = 0 for different bins of stellar (M_∗) and baryonic (M_b) mass. Each bin is constituted by 35 galaxies of similar stellar or baryonic masses. Results are shown for V_i: V_rot (upper panels), s_0.5 (middle panels) and s_1.0 (lower panels). The kinematical indicators are estimated by evaluating the gas kinematics at different radii in the simulations: R_max (dot-dashed line), 0.5   R_bar (solid line), R_bar (dotted line) and 1.5   R_bar (dashed line).