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The Gas Temperature in the Surface Layers of Protoplanetary Disks

  • Authors: I. Kamp and C. P. Dullemond

Kamp & Dullemond 2004 The Astrophysical Journal 615 991.

  • Provider: AAS Journals

Caption: Fig. 1.

Vertical structure profile of the DZN02 disk model, which forms the basis of the models described in this paper. The contours denote the particle density ﹩\mathrm{log}\,n﹩ in steps of 1. The white dashed line shows the contour that includes 95% of the disk mass.

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