Fig. 15
GC candidates with MGC ≥ 2 × 106 M⊙ on the ρSG−MSG plane, whereρSG is the mean mass density of SG stars in an originally massive GC candidate at its half-mass radius (Reff) of SG stars. All SG stars within 57 pc from the center of a GC candidate are used to estimate Reff for SG stars of the GC. These GC candidates are formed in the models with Mdm = 2 × 1010 M⊙.
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