Fig. 13
Results for model 1l, which is the fiducial model but with icy fragmentation threshold vfrag,icy = 60 m s−1. In solid black: the pebble mass flux Ṁpeb that reachesthe snowline; in dashed black: the pebble mass flux outside the snowline that is available for planetesimal formation outside the snowline; and in dotted black the critical pebble mass flux needed for streaming instability outside the snowline, all as a function of time. The total mass in planetesimals is plotted in blue.
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