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Fig. 11


Cluster total mass Mecl versus the mass of the most massive star in the cluster, mmax. Red circles indicate the position of the stellar mass derived from the upper limit of the cluster mass function, and blue rhombi label the positions of the stellar mass estimated from the earliest observed spectra. The black solid line shows the (Meclmmax) analytical relation (Weidner et al. 2013). We use black dots to show the mass estimates reported by Chené et al. (2012, 2013) and Ramírez Alegría et al. (2014).

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