Fig. 5
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Anticorrelation between the clustering-to-binary scale in the MSDC plot and stellar density for different clouds. The data point of W51 IRS2 is taken from this work; the data point of OMC-1S is taken from Palau et al. (2018); and the data points of Taurus, Ophiucus, and Trapezium are taken from Gómez et al. (1993) and Simon (1997).
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