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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 4.

Distribution functions of key molecular species for the fiducial model in the two-dimensional space of ﹩\{{\mathrm{log}}_{10}T\}\times \{{v}_{r}\}﹩ (common logarithm of temperature and radial velocity). The mass distribution function is normalized as ﹩{d}^{2}\,m/[d{\mathrm{log}}_{10}(T/{\rm{K}})d({v}_{r}/\mathrm{km}\ {{\rm{s}}}^{-1})]﹩, i.e., mass of the species per dex-temperature per ﹩({v}_{r}/\mathrm{km}\ {{\rm{s}}}^{-1})﹩.

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