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 Letters869L47.
Provider: AAS Journals
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).