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Table 2

Binary cluster candidates.

Pair IDHR24 Cluster ΔD3D ΔVt ΔV3D ΔAge logt DM E(BV) Type Overlap
pc km s−1 km s−1 Myr mag mag
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
1 5514 Theia_117 39.25 6.53 9.63 17.80 7.74 7.19 0.12 PBC
1 1 ADS_16795 39.25 6.53 9.63 17.80 7.57 7.06 0.13 PBC
2 7 ASCC_12 43.21 0.91 16.15 69.23 8.02 11.09 0.33 TBC
2 4203 HXHWL_18 43.21 0.91 16.15 69.23 7.55 10.68 0.31 TBC
3 481 CWNU_350 41.45 0.49 5.20 58.50 8.05 10.20 0.19 TBC
3 8 ASCC_13 41.45 0.49 5.20 58.50 7.73 10.80 0.25 TBC
4 5481 Theia_13 20.07 3.11 4.14 6.93 7.13 8.16 0.09 PBC
4 10 ASCC_18 20.07 3.11 4.14 6.93 7.31 8.09 0.13 PBC
5 6925 UBC_17a 17.92 1.12 1.68 9.72 6.50 8.58 0.13 PBC
5 11 ASCC_19 17.92 1.12 1.68 9.72 7.11 7.91 0.11 PBC
... ... ... ... ... ... ... ... ... ... ... ...

Notes. Column (1): Pair IDs. Column (2): Cluster IDs from Hunt & Reffert (2024). Column (3): Star cluster names. Column (4): The 3D separation between clusters, derived from α, δ, and ϖ at the epoch J2016.0. Column (5): The tangential velocity differences between clusters. Column (6): The 3D velocity differences between clusters. Column (7): Age differences of the pair clusters. Column (8): Cluster age determined by the isochrone fit. Column (9): Distance modulus determined by the isochrone fit. Column (10): Reddening determined by the isochrone fit. Column (11): Pair classification. Column (12): Previous references. The full table is available at the CDS. Here we only show the first five BCs.

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