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PROMPT PLANETESIMAL FORMATION BEYOND THE SNOW LINE

  • Authors: Philip J. Armitage, Josh A. Eisner, and Jacob B. Simon

2016 The Astrophysical Journal Letters 828 L2.

  • Provider: AAS Journals

Caption: Figure 4.

Steady-state tracks for millimeter-sized (green curves) and centimeter-sized (blue) particles in Z–﹩{\tau }_{s}﹩ space, including the effects of turbulent particle diffusion and vapor diffusion / condensation. We assume ﹩{\dot{M}}_{p}/\dot{M}=1﹩, ﹩K={10}^{3}﹩, and the fiducial disk model. The simpler models shown in Figure 1 are plotted as the dashed lines.

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