Fig. 21.

Application of getsf to the APEX λ = 350 μm image (8″ resolution) of the NGC 6334 star-forming cloud, adopting {X|Y}λ = 30″. The top row shows the original image ℐλ and the backgrounds ℬλ{X|Y} of sources and filaments. The middle row shows the component 𝒮λ, the footprint ellipses of 91 acceptably good sources on 𝒮λD, and the component ℱλD with 26 skeletons 𝒦k2 corresponding to the scales Sk ≈ 30″. The bottom row shows the standard deviations 𝒰λ in the regularized component 𝒮λR, the flattening image 𝒬λ, and the standard deviations in the flattened component . Some skeletons may only appear to have branches because they were widened for this presentation. Intensities (in MJy sr−1) are limited in range with logarithmic color mapping, except for 𝒬λ, which is shown with linear mapping.
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