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In arXiv:1505.05181, Iocco, Pato, and Bertone analyze the consistency ofModified Newtonian Dynamics (MOND) with their compiled Milky Way data andbaryonic mass distribution models. We contribute to the discussion by feedingthe baryonic mass distribution model shown as a black line in Figure 2 of theiroriginal paper, Nature Physics 11:245, into the MOND formula assuming theso-called simple interpolation function, and directly plotting these results ontop of the compiled observational rotation curve data from their originalpaper. We find that the baryonic model using MOND with the simple interpolationfunction provides a striking fit to the rotation curve observational data withno parameter adjustments required. Our results are consistent with the findingsof McGaugh (2008) as well as with studies of external galaxies.

MOND Fit of Nature Physics 11:245 Mass Distribution Model to Rotation Curve Data