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Figure 29: The mass distribution of the Milky Way disk (left) inferred from fitting in MOND
the observed bumps and wiggles in the rotation curve of the galaxy (right) [274]. The Newtonian
contributions of the stellar and gas disk are shown as dashed and dotted lines as per Figure 13.
The resulting model is consistent with independent star count data [155] and compares favorably
to constraints on the rotation curve at radii beyond those included in the fit [494]. The prominent
feature at |