Table 2
Physical properties of NGC 2264 N, NGC 2264 S, and Collinder 95.
| NGC 2264 N | NGC 2264 S | Collinder 95 | |
|---|---|---|---|
| Central RA, Dec (°) | (100.25, 9.88)1 | (100.28, 9.53)2 | (97.788, 9.894)3 |
| Central μα (mas/yr) |
2
|
4
|
3
|
| Central μδ (mas/yr) |
2
|
4
|
3
|
| Distance (pc) |
3
|
3
|
3
|
| Expansion velocity ῡout (km/s) | ![]() |
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| Core radius rc (pc) | 0.65 | 1.40 | 1.27 |
| No. YSOs within rc | 24 | 72 | 26 |
| Half-mass radius r50 (pc) | 3.835 | 3.705 | 3.695 |
| Velocity dispersion σvl(rc) (km/s) | ![]() |
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| Velocity dispersion σvb(rc) (km/s) | ![]() |
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| Velocity dispersion σvl(r50) (km/s) | ![]() |
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| Velocity dispersion σvb(r50) (km/s) | ![]() |
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| Crossing time τcross(rc) (Myr) | ![]() |
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| Crossing time τcross(r50) (Myr) | ![]() |
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| No. YSOs with closest approach < rc | 24 | 29 | 21 |
| No. YSOs with closest approach −σ < rc | 63 | 50 | 49 |
| No. YSOs with closest approach −2σ < rc | 113 | 69 | 60 |
| No. YSOs with closest approach −3σ < rc | 132 | 81 | 61 |
Notes. See the text for a discussion of how these quantities were derived. 1 Cluster center value taken from Maíz Apellániz (2019) and adjusted (+0.05°, +0) to center accurately on the cluster core of YSOs. 2 Values taken from Maíz Apellániz (2019).3 Values taken from Cantat-Gaudin et al. (2020b). 4 NGC 2264 S central proper motion value calculated by taking the median proper motion value of all YSOs located below a declination of 9.7°. 5 Half-mass radii of each cluster calculated by taking the median distance from cluster center of all member YSOs.
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