Free Access

Fig. 1


JKS CMD of the simulated nuclear clusters after 13 Gyr of evolution for a distance of 8 kpc to the GC and an average reddening of mag. The different stellar generations that were added to the simulations can clearly be distinguished in the CMD. Stars marked in red have KS < 18.5 and are used for comparison with the density profile of resolved stars from Gallego Cano et al. (2018). The remaining stars are used to create the diffuse light profile of the simulated clusters.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.