Fig. 7
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Distribution of the mass-averaged temperature of ALMA-IMF cores (Col. 7 of Tables C.4 and C.8 published at the CDS) versus luminosity-to-mass (L/M) ratios of their protocluster (Dell’Ova et al. 2024). Neither the median temperature (large markers) measured for the cores of each protocluster nor their minimum or maximum values seem to correlate with the protocluster L/M ratio.
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