ArTéMiS imaging of the filamentary infrared dark clouds G1.75-0.08 and G11.36+0.80: Dust-based physical properties of the clouds and their clumps

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Fig. 2

Same as Fig. 1, but towards G11.36+0.80. All the contour levels start from 3σ and progress in steps of 3σ. A source from the Feng et al. (2020) sample, G11.38+0.81 P3, is labelled P3 in the Spitzer 24 µm plus ArTéMiS 450 µm image. The 24 µm dark features to the south of clump B are also indicated in this image. We call them subfilaments.

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