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Fig. 4

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Three-colour image of the interface between the Rosette molecular cloud and the H ii region around NGC 2244 (red: Herschel column density map, green: PACS 70 μm, blue: Hα). The white crosses indicate the O stars. Each spectrum in Fig. 5 is integrated inside the corresponding coloured circles. The centre and radius of each circle are chosen by taking the peak value and the extension of the CO emission. The white dashed line is an indication for the separation between the pillar and globule zones.

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