Table 5.
Separation in space and velocity of binary candidates from the literature, computed from our mean parameters for 861 OCs.
| Cluster 1 | Cluster 2 | ref | Δpos (pc) | ΔV (km s−1) |
|---|---|---|---|---|
| Alessi 13 | Mamajek 1 | 1 | 92.5 | 5.1 |
| Alessi 21 | NGC 2422 | 1 | 120.8 | 9.3 |
| Platais 8 | IC 2602 | 1 | 35.9 | 4.3 |
| Turner 9 | ASCC 110 | 1 | 275.6 | 9.0 |
| Collinder 394 | NGC 6716 | 1 | 11.4 | 13.8 |
| IC 1396 | NGC 7160 | 1 | 87.6 | 13.9 |
| NGC 869 | NGC 884 | 2 | 19.5 | 19.9 |
| NGC 5617 | Trumpler 22 | 3 | 79.8 | 10.4 |
| IC 4756 | NGC 6633 | 4 | 82.9 | 8.0 |
References. (1) Conrad et al. (2017), (2) Messow & Schorr (1913), (3) De Silva et al. (2015), (4) Casamiquela et al. (2016).
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