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Fig. 8

image

Top: surface number density of the dense cores identified from the 3 mm ALMA continuum data. The white contours show the Herschel-derived column densities at N(H) = { 60,80,100,120,140 } × 1021 cm-2 (Stutz & Kainulainen 2015). Bottom: two-point correlation function of the 43 dense cores, derived with a smoothing function with FWHM = 20″ = 8400 AU.

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