![]() |
Figure 23: Residuals of MOND fits to the rotation curves of 78 nearby galaxies (all data to which
authors have access) including about two thousand individual resolved measurements. Data for 21
galaxies are either new or improved in terms of spatial resolution and velocity accuracy over those
in [401]. More accurate points are illustrated with larger symbols. The histogram of residuals is
plotted on the right panel, and is well fitted by a Gaussian of width |