Gas and stellar kinematics comparison. First column: radial profile of the inclination-corrected velocity amplitude for the stellar, ionised (Brγ), partially ionised ([Fe II]), and hot molecular gas (H₂1-0 S(1)) phases in black, blue, green, and red, respectively. Second and third columns: ring-averaged radial profiles for the velocity dispersion and the V/σ ratio. Dotted vertical lines mark the distance (i.e. R_r) adopted to extract the kinematic values from Table 5. Dashed horizontal lines in the right panels mark the V/σ = 1 value, which is commonly adopted to discriminate between rotation- and dispersion-supported galaxies.