Rotation curves V(r) for individual galaxies with good data (filled circles) together with those inferred for the dark matter halo V_h(r) after subtraction of the baryonic component (open circles). The case of ﹩Q=1﹩ is illustrated here. All plots have (0, 0) at the bottom left corner. Tick marks are 1 kpc along the abscissa and 10 km s⁻¹ along the ordinate. Galaxies are arranged in order of decreasing velocity, from ﹩V_{\mathrm{max}\,}\approx 300﹩ km s⁻¹ for NGC 5533 to ﹩V_{\mathrm{max}\,}\approx 50﹩ km s⁻¹ for DDO 154. There is a wide variety in V_h(r), ranging from nearly hollow halos to those that dominate down to small radius.