Notes. Globular clusters modeled in this paper. The half-mass radius and galactocentric distances, R_G, are taken from Harris (1996). The values of the external acceleration are calculated from with M = 1.2 × 10¹¹ M_⊙ for all galactocentric distances. Cluster masses, M_c, were calculated from the absolute V-band luminosities by assuming a stellar mass-to-light ratio of M/L_V = 2, which is close to the measured average mass-to-light ratio of galactic GCs (Mieske et al. 2008). σ_M and σ_N are the corresponding MONDian and Newtonian values of the velocity dispersion, respectively. The last column is the minimum number of stars necessary to obtain P ≤ 0.05.