Figure 3 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 3.

Deviation from the Keplerian velocity δv_rot (the upper panel) and the normalized disk surface density (the disk density over the initial disk density, the lower panel) across the gap for model h5am4p4. In the upper panel, the directly measured δv_rot is plotted as the orange curve, while the δv_rot derived from the radial force balance is plotted as the blue curve.

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