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. 2015 Oct 28;112(46):14180–14185. doi: 10.1073/pnas.1513364112

Fig. S1.

Fig. S1.

The cumulative mass distribution of objects at the end of pebble accretion (i.e., at 1 Mya) in three simulations that are identical except for α. These runs have fpl=0.004, s=50100 km, and τ=0.025 (our smallest value). Three values of α were studied; α=3×104 (our fiducial value; black curve), 105 (cyan curve), and 105 (red curve). Note that all three curves are basically identical.