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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 3.

Time evolution of gap depths measured in hydrodynamic simulations, defined as the ratio between the gas surface density at the gap center (Σgas) to the initial surface density at that location (Σgas,0). The color curves show the depth of the three gaps for the α = 5 × 10−5 model: (blue) the primary gap at 20 au, (green) the secondary gap at ∼8 au, and (red) the tertiary gap at ∼4 au. The black curve shows the depth of the primary gap (at 20 au) for the α = 5 × 10−4 model.

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