The emergence of the MD − Ṁ* correlation in the magnetohydrodynamic wind scenario

Open Access

Fig. 11

Disk fraction as a function of the cluster age (data from Fedele et al. 2010 and references therein), with the fit of the CCDF of t_disp. From the fit, we obtain t_disp = 2.37 Myr and $σ_{t_{disp}} = 0.37$ ${\sigma _{{t_{{\rm{disp }}}}}} = 0.37$ dex.

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