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Fig. 15


Period versus mass distributions for clusters with an age ranging from 4 to 150 Myr. The clusters’ name and age are given in each panel. Red dotted lines are drawn at periods of 0.2 and 10 days to guide the eye. References: Cep OB3b: Littlefair et al. (2010); NGC 2362: Irwin et al. (2008a); NGC 2547: Irwin et al. (2008b); Pleiades: Hartman et al. (2010); M 50: Irwin et al. (2009); NGC 2516: Irwin et al. (2007b); M35: Meibom et al. (2009).

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