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Fig. 5
Left: power spectra of the column density maps of the Chamaeleon clouds, which were determined from the Herschel images reprojected to a common 6′′/pixel grid (see Sect. 3.1). Right: the Δ-variance spectra of the same column density maps. The dotted vertical line indicates the resolution limit of 36′′.
This figure is made of several images, please see below:
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