Fig. 1
Two-dimensional profiles of gas density, UV flux, dust temperature, and gas temperature for our fiducial model: a 10−2 M⊙ disk with ψ = 0.2, hc = 0.1 surrounding a T Tauri star. The UV flux is plotted in units of the mean interstellar radiation field (G0, Draine 1978). Temperature only shows a limited range to highlight the cold outer disk region.
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