Bar-perturbed velocity fields obtained with our epicyclic perturbation models applied to our best fit Bertola stellar rotation curve (see text), on varying the bar pattern speed (left to right; Ω in units of km s⁻¹ kpc⁻¹) and the dimensionless damping parameter (top to bottom; λ). The FOV of each image is 12″ × 12″ and major tick marks are shown every 1″. All velocities follow the same color bar shown on the top.