Table 3: YSO evolutionary stages as defined by Robitaille et al. (2006).

Stage
Components $M_{\rm disk}/M_\star$ $\dot{M}_{\rm env}/ M_\star$

I
accreting envelope any > $10^{-6} \ {\rm yr}^{-1}$
II disk, remains of envelope >10-6 < $10^{-6} \ {\rm yr}^{-1}$
III optically thin disk <10-6 < $10^{-6} \ {\rm yr}^{-1}$


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