Table D.1
Mass segregation results with ΛMSR method (based on Allison et al. 2009) in various core clusters of NGC 2068 and 2071.
| N = 2 | N = 3 | N = 5 | N = 10 | |
|---|---|---|---|---|
| N11 | 0 | 0 | ||
| N1 | 0 | 0 | ||
| N2 | 4 | 2 | 2 | |
| N22 | 0 | 0 | ||
| N211 | 0 | 0 | ||
| N212 | 0 | 1 | 0 | |
| N0 (N1+N2) | 0 | 1 | 2 | |
| N22+N211 | 1 | 1 | 0 | |
| robust pre >2 × 1021 cm−2 | 0 | 2 | 3 | |
| cand. pre >2 × 1021 cm−2 | 0 | 2 | 3 |
Notes. This table summarizes results on mass segregation using various core samples that are listed in the left column (see Fig. D.2 and text for details). The assigned numbers in the table from 0 to 4 correspond to a range of No to Strong in properties of mass segregation. In a given cluster we analyzed the spatial distribution of cores against the N = 2, 3, 5, 10 highest mass cores in that cluster, provided that this was reasonable based on the size of the cluster (table cells are empty if not).
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