Аннотация:Rotation curves for the inner regions of NGC 4357, 4814, and 5371 were obtained from spectral observations with the 6-m telescope of the Special Astrophysical Observatory of the USSR Academy of Sciences. The bulge-to-disk mass ratios appear to be very different for the galaxies; and the contribution of the dark halo to the integral inner-part mass appears to be insignificant for all the galaxies.