Fig. 6.

High-resolution surface densities obtained for the Herschel images of Cygnus X (HOBYS project, Motte et al. 2010; Hennemann et al. 2012; Bontemps et al., in prep.). The top row shows the hires surface densities 𝒟OH from Eq. (8) with OH = 18.2″ and 5.9″ resolutions, and the high-contrast from Eq. (10) with OH = 5.9″. The bottom row displays the relative differences of 𝒟18″, 𝒟12″, and 𝒟6″ with respect to the next lower-resolution surface densities 𝒟25″, 𝒟18″, and 𝒟12″, respectively. Logarithmic and square-root color mapping in the top and bottom rows, correspondingly.
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