Table A.2
p-values resulting from applying a two-sample K-S test to the distributions in mass of Class II and Class III objects projected onto each of the six NGC 2264 subregions shown in Fig. 10.
| Field | Halo | Cone (H) | S Mon | Cone (C) | Spokes | |
|
|
||||||
| M⋆(M⊙) [Class II] | 0.76 | 0.55 | 0.70 | 0.65 |
0.59 |
0.66 |
| M⋆(M⊙) [Class III] | 0.63 |
0.52 |
0.51 |
0.73-0.01 | 0.50 |
0.96 |
| p-value | 0.869 | 0.520 | 0.535 | 0.226 | 0.942 | 0.434 |
Notes. The upper and lower error bars associated with the median masses delimit the range of variability of the computed median if we take into account the objects with (Teff, Lbol) coordinates but no mass estimate from the HR diagram in Fig. 7 because they fall outside the area covered by the model grid. When no error bars are reported, the variation on the value estimated following this approach is lower than 0.01.
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