Fig. 3
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Distribution of St = 1 solid material in the vicinity of an 1 M⊙ planet in BR and NBR models assuming η = 0 (panels A), η = 0.1 (panels B), and η = 1 (panels C) with p = 0.5. The density ratio of the BR and NBR models are also shown on the left. The circles represent the planetary Hill sphere. The axes are shown in code units.
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