Fig. 2.

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Rotation curves for the McM model (left panel) and the PW model (right panel). The solid lines show the components for the Newtonian framework. All dashed lines correspond to the MOND framework. The horizontal dotted black line shows the MONDian asymptotic velocity of the velocity curve, , where Mbary is the total baryonic mass. The dot shows the circular velocity at the solar radius from McMillan (2017). The baryonic models in the Newtonian and MOND framework have the same parameters, except for the increased disk mass in the MOND framework, which is needed to fit Vc(R⊙).
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