Figure 20

Figure 20: Comparison of theoretical rotation curves for the inner parts (before the rotation curve flattens) of an HSB exponential disk [145], computed with three different formulations of MOND. Green: Milgrom’s formula; Blue: Bekenstein–Milgrom MOND (AQUAL); Red: TeVeS-like multi-field theory. Image reproduced by permission from [145], copyright by APS.