Fig. 9
Mass-radius distributions of Gaussian fragments extracted from Gaussclumps. The masses are listed in Table 1 and the effective radius is derived with 
. The red line delineates the threshold introduced by Kauffmann & Pillai (2010) separating the regimes under which high-mass stars can form (above the line) or not (below the line). The green and blue points belong to αvir< 1 and αvir> 1, respectively.
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