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Diverse Protoplanetary Disk Morphology Produced by a Jupiter-mass Planet

  • Authors: Jaehan Bae, Paola Pinilla, and Tilman Birnstiel

2018 The Astrophysical Journal Letters 864 L26.

  • Provider: AAS Journals

Caption: Figure 7.

Time evolution of dust-to-gas mass ratio Σgraingas at the peak of the dust rings. The black and red curves show the Σgraingas values at the peak of dust rings in Models 1 and 2: (dotted) the inner ring at ∼5 au, (dashed) the middle ring at ∼11 au, and (solid) the outer ring at ∼32 au. The blue solid curve shows the Σgraingas value at the peak of the outer dust ring in Model 3 at ∼29 au.

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