Fig. 5

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Comparison of the optical depth, τ, of dust (black solid lines) to that of para- and ortho-H2 (blue and cyan solid lines, respectively, upper-left panel), H (orange solid lines, upper-right panel), CO (green solid lines, bottom-left panel), and N2 (purple solid lines, bottom-right panel) at N(H2) = 1021 cm−2. The H2 optical depth is shown for model ℋ and H2 o:p = 3:1. The H, CO, and N2 optical depths have been computed by assuming constant abundances and the photoabsorption cross sections presented in the Leiden Observatory database (https://home.strw.leidenuniv.nl/~ewine/photo/; see also Heays et al. 2017).
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