Fig. 6
Menv − Lbol diagram of the sources in the ℓ = 30° (left panel) and ℓ = 59° (right panel) fields for the prestellar and protostellar cores shown in Fig. 2. The solid black line and the dashed black line are the best log-log fit of the high-mass counterparts of the Class I and Class 0 sources, respectively, in the low-mass regime, as found in Molinari et al. (2008).
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