Fig. 10

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Mean intensity, Jv, of the total emission in the wavelength range 72 < λ/nm < 250 for a molecular cloud illuminated by one side. From top to bottom the four panels show the expected mean intensity from H2 lines, H2 continuum, H lines (Lyα and Lyβ), and ISRF at four different column densities, from N = 1021 to 4 × 1022 cm−2. Insets show the components of Jv at 400 < λ/nm < 700, highlighting three lines of the Balmer series (Hα, Hβ, and Hγ). Results are shown for model ℋ, χ = 1, H2o:p=0:1, and Rv = 3.1.
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