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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. 7.

Abundances of selected species in the standard disk model: H, H2, C, C﹩^{+}﹩, CO, CH, OH, and CH2. See Fig. 2 for the meaning of the overplotted lines. The colors correspond to logarithmic abundances in steps of 1 and range from ﹩\mathrm{log}\,\epsilon =-14﹩ to 0.

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