Table 1
Cluster parameters for selected open clusters.
| Cluster | Nstars | α | δ | μα* | μδ | ϖp | log(age) | Z | AV | m − M |
|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (mas yr−1) | (mas) | (dex) | (mag) | ||||||
| … | ||||||||||
| BH 99 | 544 | 159.49 | −59.15 | −14.46 | 1.00 | 2.207 | 7.66 | 0.0672 | 0.34 | 8.35 |
| Collinder 463 | 644 | 27.06 | 71.74 | −1.74 | −0.37 | 1.123 | 8.51 | 0.1943 | 0.79 | 9.65 |
| IC 1396 | 577 | 324.80 | 57.53 | −2.26 | −4.58 | 1 . 040 | 6.98 | −0.0225 | 1.59 | 9.79 |
| Melotte 22 | 1130 | 56.61 | 24.10 | 19.92 | −45.40 | 7.322 | 8.01 | 0.0287 | 0.17 | 5.55 |
| NGC 1342 | 455 | 52.91 | 37.39 | 0.41 | −1.66 | 1 .485 | 9.05 | −0.1134 | 0.71 | 9.18 |
| … | ||||||||||
Notes. Equatorial coordinates (α, δ), proper motions (µα*, µδ), and corrected parallax (ϖP) are computed as the median values in each cluster sample. The cluster parameters log(age), Z, AV, and m − M are estimated through the BASE-9 suite software. The full version of this table is available at the CDS.
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