Fig. 12.
Logarithmic Ṁacc vs. disk mass distribution for stars in the TWA, compared to the populations of the Lupus and Chamaeleon I star-forming regions. The straight lines mark the Ṁacc − Mdisk relationship predicted for different stellar ages in a scenario of viscous quasi-steady disk evolution (Rosotti et al. 2017). Upper limits are indicated by correspondingly oriented arrows.
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