Fig. 21.
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Assessment of mass segregation in NGC 2244. Left: cumulative distributions of mass as a function of the projected distance from the NGC 2244 centre. The masses are divided at 1 M⊙. The confidence intervals correspond to 1σ. Right: mass segregation ratio, ΛMSR as a function of the NMST stars. The horizontal dashed line indicates ΛMSR = 1, corresponding to no mass segregation.
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