Fig. 9
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Similar to Fig. 6 but in the fragmentation-limited disk. The stokes number is inversely related to the turbulence strength, and we adopt τs = 0.05 when αt = 10−3. The parameters are listed in Table 2. The giant planet formation region is significantly narrower compared to the one depicted in Fig. 6, primarily because the growth of pebble size is suppressed in high-turbulence disks.
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