Fig. 16.
Properties of the first Larson core when ρg ∼ 10−11 g cm−3 for Col1, Col10, and Col100. The core mass, the dust mass ratio, and the formation time are shown as a function of the grain size (blue circles). The results are compared with the fiducial ColGAS simulation (dashed red lines). The top x-axis shows the initial Stokes number in the core St0.
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