Fig. 2
As Fig. 1, but for the YOC candidate members. The clusters with ages ≤50 Myr are compared with literature data from IC 2391 (Randich et al. 2001), IC 2602 (Randich et al. 1997, 2001), and IC 4665 (Martin & Montes 1997; Jeffries et al. 2009a), while the NGC 2451A cluster has been compared with data from Alpha Persei (Balachandran et al. 2011) and from NGC 2451A itself (Hünsch et al. 2004).
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