Figure 2 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 2.

Azimuthally averaged gas surface density for models of h/r = 0.05, 0.07, and 0.1 are shown from left to right. Disks with α = 10⁻⁴, 10⁻³, 10⁻² are shown from top to bottom. Blue, yellow, green, red, and purple curves represent the gas surface density for planet masses M_p = 11 M_⊕, 33 M_⊕, 0.3 M_J, 1 M_J, and 3 M_J, respectively, if M_* = M_⊙. The dashed curves show the cases with visible asymmetry at the gap edge in Figure 1.

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