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Fig. 9


Spatial variations of the amount of reddening per gas nucleon, /NH γ, with the total gas measured by NH γ at 0. °375 resolution (top panel) and its variations relative to the average value of (2.02 ± 0.48) × 10−22 mag cm2 (bottom panel). Quantities with a tilde are convolved with the LAT response for an interstellar spectrum. The black contours outline the shape of the CO clouds at the level of 1 K km s−1 in WCO intensity.

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