Ratio between values of the stellar specific angular moment obtained when the asymmetric drift correction is applied (j_*) or not (j_*, no AD), i.e. co-rotation if stars and gas is assumed, as a function of M_*. Orange points show the ratios for each galaxy, while the dashed black and blue lines show the median of the distribution and the running mean, respectively. Three galaxies have a larger j_* when the asymmetric drift correction is applied. This is because those galaxies have a strong contribution of pressure-supported motions, such that the stellar rotation curve derived from the circular speed profile has a larger amplitude than the H I rotation curve.