Table 3
Distribution of periodic sources among the various NGC 2264 subregions.
| Cone (H) | S Mon | Halo | External | |
|
|
||||
| Full sample | 29.8% | 28.0% | 27.8% | 14.4% |
| Periodic | 30.9% | 29.8% | 29.1% | 10.2% |
| P[1,2] | 38.5% | 25.6% | 28.2% | 7.7% |
| P[3,4] | 22.7% | 27.3% | 34.1% | 15.9% |
Notes. Each column corresponds to a different subclustering identified in the NGC 2264 region by Sung et al. (2009) and illustrated here in Fig. 15. Rows indicate, in the order, the percentage of objects located on top of each of the subregions among (i) the full sample investigated in this study; (ii) objects found to be periodic (single period) in this study; (iii) periodic sources with period between 1 and 2 days; and (iv) periodic sources with period between 3 and 4 days. The percentage indicated for Cone (H) also accounts for objects projected onto Cone (C) and onto the Spokes region.
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