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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 1.

Normal inner and outer Lindblad torques for various values of the disk thickness H/ r evaluated including the effect of the pressure buffer (see W97), and normalized by the value T o ≡ ( M p / M *) 2Σ r 4Ω 2( H/ r) −3 evaluated at the planet location, where M * is the mass of the host star. The torques are cut off for m > Δ m cutoff∝( H/ r) −1.

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