Figure 7 from The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet

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The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet–Disk Interactions Interpretation

Authors: Shangjia Zhang, Zhaohuan Zhu, Jane Huang, Viviana V. Guzmán, Sean M. Andrews, Tilman Birnstiel, Cornelis P. Dullemond, John M. Carpenter, Andrea Isella, Laura M. Pérez, Myriam Benisty, David J. Wilner, Clément Baruteau, Xue-Ning Bai, and Luca Ricci

2018 The Astrophysical Journal Letters 869 L47.

Caption: Figure 7.

Similar to Figure 6, except that the initial dust size distribution is assumed to follow n(s) ∝ s^−2.5 with the maximum grain size of 1 cm (DSD2).