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This article has an erratum: [https://doi.org/10.1051/0004-6361/202243556e]


Fig. 5.

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Value of the present-day slope of the stellar mass function (αpd) plotted as a function of the ratio (log(tage/trh)), where tage are the ages of the clusters and the th their present-day half-mass relaxation time (upper subpanel) and fraction of G1 stars in the clusters plotted as a function of log(tage/trh) (lower subpanel). In both subpanels, clusters are segregated by their mass, which is taken to be the mean value of the photometric and dynamical masses.

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