  In arXiv:1505.05181, Iocco, Pato, and Bertone analyze the consistency of
Modified Newtonian Dynamics (MOND) with their compiled Milky Way data and
baryonic mass distribution models. We contribute to the discussion by feeding
the baryonic mass distribution model shown as a black line in Figure 2 of their
original paper, Nature Physics 11:245, into the MOND formula assuming the
so-called simple interpolation function, and directly plotting these results on
top of the compiled observational rotation curve data from their original
paper. We find that the baryonic model using MOND with the simple interpolation
function provides a striking fit to the rotation curve observational data with
no parameter adjustments required. Our results are consistent with the findings
of McGaugh (2008) as well as with studies of external galaxies.
