Rotation curves of 32 mainly HSB galaxies. The points with vertical error bars are the observed data. The dotted (black) and short dashed lines are contributions of the gaseous and stellar components to the Newtonian rotation speeds, respectively. The long dashed (blue) line is that of MOND1. The solid line is the rotation curve constructed through MOND3. The M_∗/Ls of MOND3 are used in plotting the stellar component. The dashed-dotted (green) and dotted (red) lines are those of the MOG and NFW models, respectively.