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Fig. 3.

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Models with G0 = 2 × 104 and different values of nH and xC . Red and blue markers show the predicted C0 column density and [C I] 609 μm intensity, respectively, from AV = 0 to 10 mag into the wind and disk system. The gas density derived from H2 observations is ≈107 cm−3 (Berné et al. 2024). The horizontal line marks the observed intensity (±1σ). Circles and triangles represent models with small depletion factors of two and three, respectively.

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