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Fig. 8

image

XCO map of the mIVC at the locations of detected 12CO(1 0) emission. The contours mark the modelled dust optical depth from Planck from 1 × 10-6 to 9 × 10-6 in steps of 2 × 10-6. The values range between 0.5 × 1020 cm-2 (K km s-1)-1XCO ≲ 11 × 1020 cm-2 (K km s-1)-1. We note that the XCO map is derived at the angular resolution of the Planck data, which is shown at the bottom-left.

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