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Fig. 9

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Integrated colours of open clusters vs. cluster age. The left panel shows data for (B − V), the right one for (J − Ks). The observations of the Galactic open clusters are indicated by dots, blue for MS-clusters, green for post-MS clusters, and red for RG-clusters (see Sect. 2 for explanation). Bars in the upper-right corner of each panel mark typical errors of the integrated colours. The solid curves are evolutionary tracks of a SSP model with a continuous IMF for a cluster with Mc = 103   m and ml = 0.1   m. The connected symbols (crosses) show the discrete-IMF option of this model.

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