Fig. 1.
Time evolution of the system of RUN1: (a) t = 0, (b) t = 29.4 TKep, (c) t = 1.47 × 103 TKep, and (d) t = 2.94 × 104 TKep, where TKep is the Keplerian period at r = aR. The green point is the outer satellite and the purple dots show the disk particles. The inner and outer circles in black solid lines represent the planetary surface and the Roche limit (r = aR).
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