Fig. 1
Relation between accretion rates derived from the hydrodynamical simulations (at an age of 1 Myr) and stellar mass for the cold (blue dots) and hybrid (magenta squares) cases. The magenta crosses are taken from the observations of Venuti et al. (2014). The dashed lines indicate the lower and upper limits observationally derived by Fang et al. (2013).
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