Fig. A.1

Dust temperature as a function of optical depth of a molecular clouds which are illuminated by an interstellar radiation field (ISRF) of (10,100,1000) times the Galactic ISRF at the solar radius (plus signs). The solid line for τV ≤ 10 and dashed line for τV> 10 correspond to Tdust ∝ (I/I(0))1/5.5. The solid line for τV> 10 corresponds to I/I(0) = 0.246.
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