Table 4.
Fundamental parameters and parallax distances obtained for the confirmed and probable clusters.
| Cluster | z | Age | E(B − V) | Mass | dASteCA | dnoofset | dLindegren | dSchönrich | dXu |
|---|---|---|---|---|---|---|---|---|---|
| (109 yr) | mag | (103 M⊙) | (kpc) | (kpc) | (kpc) | (kpc) | (kpc) | ||
| vdBH 73 | 0.019±0.004 | 0.78±0.09 | 1.06±0.04 | 2.6±0.9 | 5.01 ± 0.61 | 5.48 ± 0.44 | 4.92 ± 0.41 | 4.46 ± 0.31 | 4.05 ± 0.33 |
| RUP 85 | 0.021±0.003 | 0.18±0.03 | 1.06±0.03 | 2.6±0.5 | 4.80 ± 0.26 | 5.39 ± 0.23 | 4.64 ± 0.19 | 4.16 ± 0.15 | 3.83 ± 0.14 |
| vdBH 85 | 0.014±0.002 | 7.50±0.80 | 0.30±0.03 | 2.2±0.5 | 4.61 ± 0.26 | − | 4.15 ± 1.38 | − | − |
| vdBH 87 | 0.025±0.002 | 0.25±0.08 | 0.55±0.04 | 1.4±0.2 | 2.08 ± 0.09 | 2.42 ± 0.07 | 2.26 ± 0.06 | 2.13 ± 0.05 | 2.05 ± 0.05 |
| TR 12 | 0.009±0.002 | 0.70±0.10 | 0.31±0.03 | 0.7±0.1 | 3.50 ± 0.15 | 4.08 ± 0.14 | 3.63 ± 0.13 | 3.31 ± 0.10 | 3.11 ± 0.09 |
| vdBH 92 | 0.009±0.004 | 0.02±0.01 | 0.65±0.03 | 0.4±0.1 | 2.59 ± 0.11 | 2.61 ± 0.11 | 2.43 ± 0.09 | 2.28 ± 0.07 | 2.17 ± 0.07 |
| TR 13 | 0.007±0.004 | 0.11±0.02 | 0.56±0.02 | 0.7±0.2 | 4.81 ± 0.33 | 5.25 ± 0.16 | 4.58 ± 0.14 | 4.10 ± 0.11 | 3.75 ± 0.09 |
| vdBH 106* | 0.012±0.003 | 3.00±0.80 | 0.30±0.04 | 0.5±0.2 | 4.87 ± 0.81 | 5.41 ± 0.39 | 4.77 ± 0.39 | 4.31 ± 0.33 | 4.06 ± 0.30 |
| RUP 162* | 0.009±0.002 | 0.80±0.20 | 0.54±0.03 | 1.2±0.2 | 4.43 ± 0.20 | 4.97 ± 0.20 | 4.37 ± 0.18 | 3.94 ± 0.15 | 3.66 ± 0.13 |
| NGC 4349 | 0.011±0.004 | 0.29±0.09 | 0.41±0.05 | 2.0±0.1 | 1.88 ± 0.05 | 2.04 ± 0.03 | 1.92 ± 0.02 | 1.83 ± 0.02 | 1.76 ± 0.01 |
Notes. The asterisk indicates probable clusters. The dnoofset values are those obtained using the Bayesian method without bias correction on the Gaia DR2 parallax data. The remaining distances were obtained by applying the indicated offsets to the parallax values.
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