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Fig. 14

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Comparison between the H2CO distribution with that of τ353, NHI, and 13CO. The spatial distribution of τ353 is derived from the Planck measurements (top), the HI column density from EBHIS (Winkel et al. 2016), and the13 CO (1−0) integrated intensity from Schneider et al. (2011) at an angular resolution of 10.8. In all panels, the contours correspond to the smoothed integrated optical depth map of H2CO (11,0−11,1) integrated from −10 km s−1 to 20 km s−1, and they start from 0.09 km s−1 and increase by 0.09 km s−1. The SSI (see Sect. 6.3) of the two corresponding tracers is indicated in the lower left corner of each panel.

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