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Fig. 2


Colour–magnitude diagrams of different regions of the simulated stellar system obtained from MICADO simulations. The lines are the isochrones from Marigo et al. (2008) representative of the nuclear cluster stars. The red line is the MS and the RGB, while the blue line is the sequence of core He-burning stars, up to the first thermal pulse on the AGB. The upper-left sub-panels show the CMDs of the input stellar catalogues (NSC plus host galaxy main body). For clarity only stars in the inner 3re region are shown.

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