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Hydrodynamic Photoevaporation of Protoplanetary Disks with Consistent Thermochemistry

  • Authors: Lile Wang and Jeremy J. Goodman

2017 The Astrophysical Journal 847 11.

  • Provider: AAS Journals

Caption: Figure 8.

Radial profiles of the differential wind mass-loss rate, ﹩(2\pi {R}^{2}\dot{{\rm{\Sigma }}})﹩, for the time-averaged fiducial simulation. Dashed curve is calculated by applying GH09's prescription to the density and temperature structure of our simulation, whereas solid curve is our actual mass-loss rate.

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