Fig. 14
-Reff
distributionsof all continuum and NH2D cores. The masses are derived from the integrated flux within a measured Gaussian FWHM using GAUSSCLUMPS, and the effective radius is 
. The dashed gray line shows a threshold between high-mass and low-mass star candidates (Kauffmann & Pillai 2010). The yellow and other color points indicate the continuum and NH2D cores, respectively.
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