Fig. 10.
Left panel: RAR at 1 kpc with the L18a parameters. Observational errors from the rotation curve measurements are also plotted. The large errors seem to be associated with a downward scatter in gobs with respect to the RAR. Right panel: RAR at 5 kpc. The observational errors are small and the RAR is particularly tight at this radius. The six representative galaxies in Fig. 6 are displayed as in Fig. 9.
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