Fig. F.5
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As Fig. 15 but for the case of lower column density N(H2) = 3 · 1022cm−2, higher background surface brightness Ibg=100 MJy sr−1 and the model filament illumination by an isotropic radiation field only (χ=1). The observed surface brightness is assumed to consist only of the extincted background and thermal dust emission from stochastically heated grains.
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