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Protoplanetary Disk Resonances and Type I Migration

  • Authors: David Tsang

Tsang 2011 The Astrophysical Journal 741 109.

  • Provider: AAS Journals

Caption: Figure 2.

Resonant gain Γ m for the first three azimuthal modes for linear viscous damping with H/ r = 0.05 and α = 10 −3. Far from the disk edge Γ m → 1. The gain increases strongly for waves that are resonant in the disk.

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