Figure 9 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.

Provider: AAS Journals

Caption: Figure 9.

Contrast at the outer gap edge for every model. The upper panels use DSD1 dust size distribution while the lower panels use DSD2 dust size distribution. Contrast is the intensity of the brightest part of the ring over the intensity at Δθ = 180° opposite location on the ring.

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