Molecular cloud matching in CO and dust in M33 - I. High-resolution hydrogen column density maps from Herschel

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Fig. 6.

(N_{H, Method I} − N_{H, Method II})/N_{H, Method II} difference map of the dust-derived total column density maps. The grey ellipse roughly delineates the area of enhanced emission observed in the western half of M33, as depicted in Figs. 3 (left) and 4 (left), in contrast to the eastern half.

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