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Table 1
Main properties of the clusters investigated in this work according to Cantat-Gaudin et al. (2020): radius containing half of the members (r50), number of high-probability members (N), age (log τ), extinction (AV), and average distance (d).
| Cluster | r50 (°) | N | log τ | AV | d (pc) |
|---|---|---|---|---|---|
| Melotte 20/α Per | 2.027 | 747 | 7.71 | 0.30 | 171 |
| Pleiades/Melotte 22 | 1.274 | 952 | 7.89 | 0.18 | 128 |
| ASCC 16(*) | 0.376 | 175 | 7.13 | 0.20 | 344 |
| ASCC 19 | 0.605 | 149 | 7.02 | 0.13 | 346 |
| NGC 2232 | 0.516 | 188 | 7.25 | 0.01 | 315 |
| Roslund 6 | 1.004 | 247 | 7.95 | 0.00 | 375 |
| NGC 7058 | 0.109 | 26 | 7.61 | 0.18 | 350 |
| ASCC 123 | 1.294 | 49 | 7.65 | 0.00 | 229 |
Notes. (*)Identified as Briceno 1 in Hunt & Reffert (2023) and Cavallo et al. (2024).
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