Table A.2
Kinematic and physical parameters of cluster pair candidates.
| ClusterCG20 | ClusterH&R24 | Δ3D pc | RVCG20 km·s−1 | NCG20 | RVH&R24 km·s−1 | NH&R24 | TVCG20 km·s−1 | TVH&R24 km·s−1 | logAgeCG20 dex | logAgeH&R24 dex |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| UBC_207 | NGC_1980 | 10.61 | 22.12±10.62 | 24 | 23.24±2.84 | 93 | 2.17±0.25 | 2.46±0.01 | 7.18 | ![]() |
| UBC_420 | Berkeley_65 | 48.13 | -64.24±1.62 | 1 | -60.43±7.02 | 1 | 7.64±0.76 | 8.78±0.08 | 7.81 | ![]() |
| NGC_2645 | Pismis_8 | 32.93 | -25.27±4.52 | 2 | - | 0 | 67.75±1.03 | 67.06±0.22 | 7.41 | ![]() |
| UBC_468 | Ruprecht_35 | 49.25 | 44.05±0.23 | 1 | - | 0 | 75.50±3.75 | 73.87±0.55 | 7.04 | ![]() |
| SAI_72 | CWNU_1966 | 37.41 | 44.56±1.26 | 1 | 33.76±21.68 | 2 | 9.04±0.91 | 17.43±0.26 | - | ![]() |
| UBC_14 | ASCC_106 | 34.10 | -6.28±7.45 | 22 | -15.38±1.81 | 20 | 7.71±0.28 | 9.39±0.11 | 7.72 | ![]() |
| UPK_533 | UPK_535 | 31.26 | 27.12±3.70 | 17 | 3.91±4.45 | 25 | 11.91±0.33 | 20.24±0.06 | 7.95 | ![]() |
| NGC_1977 | ASCC_19 | 43.86 | 25.38±7.68 | 31 | 11.65±3.37 | 26 | 2.84±0.42 | 2.81±0.03 | 7.99 | ![]() |
| NGC_1977 | HSC_1633 | 25.16 | 25.38±7.68 | 31 | 14.80±5.66 | 17 | 2.84±0.42 | 3.82±0.03 | 7.99 | ![]() |
| NGC_1977 | OC_0339 | 43.00 | 25.38±7.68 | 31 | 29.10±7.32 | 3 | 2.84±0.42 | 3.37±0.03 | 7.99 | ![]() |
| NGC_1977 | OCSN_59 | 48.91 | 25.38±7.68 | 31 | 17.39±4.30 | 13 | 2.84±0.42 | 2.71±0.04 | 7.99 | ![]() |
| NGC_1977 | Sigma_Orionis | 17.53 | 25.38±7.68 | 31 | 24.97±4.15 | 31 | 2.84±0.42 | 3.05±0.05 | 7.99 | ![]() |
| NGC_1977 | UBC_17a | 38.63 | 25.38±7.68 | 31 | 11.74±3.44 | 35 | 2.84±0.42 | 3.80±0.02 | 7.99 | ![]() |
| UBC_392 | CWNU_446 | 43.78 | -3.26±3.12 | 7 | -33.23±7.82 | 6 | 15.38±0.23 | 11.88±0.15 | 7.85 | ![]() |
| UBC_392 | CWNU_1126 | 33.10 | -3.26±3.12 | 7 | -25.15±2.73 | 17 | 15.38±0.23 | 15.60±0.11 | 7.85 | ![]() |
| UBC_392 | CWNU_1228 | 27.59 | -3.26±3.12 | 7 | -38.19±6.19 | 1 | 15.38±0.23 | 13.42±0.13 | 7.85 | ![]() |
| UBC_392 | OC_0185 | 37.78 | -3.26±3.12 | 7 | -20.23±3.23 | 54 | 15.38±0.23 | 12.37±0.06 | 7.85 | ![]() |
| UBC_672 | HSC_2848 | 31.60 | -34.47±5.48 | 1 | - | 0 | 16.46±0.70 | 13.80±0.11 | 7.02 | ![]() |
| UBC_672 | HSC_2849 | 30.86 | -34.47±5.48 | 1 | -30.33±14.88 | 3 | 16.46±0.70 | 13.06±0.10 | 7.02 | ![]() |
| UBC_672 | NGC_6231 | 13.23 | -34.47±5.48 | 1 | -30.80±4.22 | 57 | 16.46±0.70 | 17.59±0.05 | 7.02 | ![]() |
| UBC_672 | OC_0673 | 13.89 | -34.47±5.48 | 1 | -34.28±5.41 | 6 | 16.46±0.70 | 17.07±0.08 | 7.02 | ![]() |
| UBC_553 | ESO_332-13 | 31.86 | 14.91±42.96 | 2 | -18.32±6.49 | 18 | 15.44±0.64 | 9.27±0.09 | 7.12 | ![]() |
| UBC_553 | HSC_2849 | 10.16 | 14.91±42.96 | 2 | -30.33±14.88 | 3 | 15.44±0.64 | 13.06±0.10 | 7.12 | ![]() |
| UBC_553 | NGC_6231 | 30.95 | 14.91±42.96 | 2 | -30.80±4.22 | 57 | 15.44±0.64 | 17.59±0.05 | 7.12 | ![]() |
| UBC_553 | OC_0673 | 42.80 | 14.91±42.96 | 2 | -34.28±5.41 | 6 | 15.44±0.64 | 17.07±0.08 | 7.12 | ![]() |
| FSR_0198 | Casado_82 | 30.43 | -9.55±4.46 | 2 | -22.38±8.49 | 1 | 72.40±3.69 | 67.34±0.31 | 6.67 | ![]() |
| FSR_0198 | Teutsch_8 | 43.79 | -9.55±4.46 | 2 | 11.42±14.31 | 3 | 72.40±3.69 | 70.50±0.27 | 6.67 | ![]() |
| Kronberger_1 | HSC_1351 | 15.90 | - | 0 | - | 0 | 23.93±1.65 | 17.91±0.24 | 6.78 | ![]() |
| Kronberger_1 | HSC_1356 | 16.99 | - | 0 | 79.41±8.86 | 1 | 23.93±1.65 | 19.37±0.15 | 6.78 | ![]() |
| Bochum_11 | ASCC_62 | 44.52 | -24.73±60.56 | 7 | 41.38±20.97 | 1 | 78.36±2.94 | 78.84±0.35 | 6.80 | ![]() |
| Bochum_11 | Collinder_228 | 18.05 | -24.73±60.56 | 7 | -28.41±14.03 | 2 | 78.36±2.94 | 82.39±0.34 | 6.80 | ![]() |
| Bochum_11 | Trumpler_16 | 32.74 | -24.73±60.56 | 7 | -2.88±13.41 | 14 | 78.36±2.94 | 87.02±0.24 | 6.80 | ![]() |
Notes. Columns (1) and (2) give the cluster names from CG20 and H&R24, respectively. Column (3) gives the three-dimensional separation (Δ3D) between the two clusters in each pair. Columns (4) and (5) report the RV of the CG20 cluster and the number of members used in its calculation. Columns (6) and (7) list the RV of the H&R24 cluster (taken directly from the catalog) and the corresponding number of members with RV measurements. Columns (8) and (9) provide the TVs of the clusters. Columns (10) and (11) present the ages of the clusters.
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