Fig. 15
NH maps (in cm-2) for the different gas phases in the analysis region: H i in the intermediate velocity arc and, inside the Chamaeleon complex, gas in the H i, DNM, and CO-bright phases. The maps are based on the γ + AVQ analysis, with the assumption of optically thin H i, the value of XCOγ, and the dust DNM template calibrated in mass with the γ rays.
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