Fig. 8
Disk fraction as a function of period obtained from model M2 (red circles) for t = 2.1 Myr (left panel) and for t = 3.1 Myr (right panel). The superimposed black circles show the disk fraction as a function of the period obtained for the ONC (left panel) and for NGC 2264 (right panel) for stars with a spectral type M2 and earlier extracted from Cieza & Baliber (2007).
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