Modified Newtonian dynamics in the Milky Way

Both microlensing surveys and radio-frequency observations of gas flow imply that the inner Milky Way is completely dominated by baryons, contrary to the predictions of standard cold dark matter (CDM) cosmology. We investigate the predictions of the modified Newtonian dynamics (MOND) formula for the Galaxy given the measured baryon distribution. Satisfactory fits to the observationally determined terminal-velocity curve are obtained for different choices of MOND's interpolating function μ(x). However, with simple analytical forms of μ(x), the local circular speed v_c(R₀) can be as large as 220kms^-1 only for values of the parameter a₀ that are excluded by observations of NGC 3198. Only a numerically specified interpolating function can produce v_c(R₀) = 220kms^-1, which is therefore an upper limit in MOND, while the asymptotic velocity is predicted to be v_c(∞) = 170 +/- 5kms^-1. The data are probably not consistent with the functional form of μ(x) that has been explored as a toy model in the framework of Bekenstein's covariant theory of gravity.