Open Access
Fig. D.4
Mass segregation ratio, ΛMSR, as function of core mass in the N2 cluster of NGC 2068 and 2071, including 100 robust prestellarcores (see left panel of Fig. D.2). The tool used to derive ΛMSR is described in Allison et al. (2009). A sliding window of three cores (N = 3) was set in this case.
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