Table 2
Basic parameters from the literature for all CAPOS clusters.
| Cluster ID | [Fe/H] | E(B-V) | Vr (km s−1) | μαcosδ (mas yr−1) | μδ (mas yr−1) | Mass (M⊙) |
|---|---|---|---|---|---|---|
| NGC 6273 | −1.74 | 0.38 | 145.54±0.59 | −3.249±0.026 | 1.660±0.025 | 7.19 ± 0.37 × 105 |
| NGC 6293 | −1.99 | 0.36 | −143.66±0.39 | 0.870±0.028 | −4.326±0.028 | 1.42 ± 0.12 × 105 |
| NGC 6304 | −0.45 | 0.54 | −108.62±0.39 | −4.070±0.029 | −1.088±0.028 | 1.03 ± 0.04 × 105 |
| NGC 6316 | −0.45 | 0.54 | 99.81±0.82 | −4.969±0.031 | −4.592±0.030 | 3.47 ± 0.44 × 105 |
| Terzan 2 | −0.69 | 1.87 | 128.96±1.18 | −2.170±0.041 | −6.263±0.038 | 8.05 ± 2.31 × 104 |
| Terzan 4 | −1.41 | 2.00 | −39.93±3.76 | −5.462±0.060 | −3.711±0.048 | 1.81 ± 0.53 × 105 |
| HP1 | −1.00 | 1.12 | 40.61±1.29 | 2.523±0.039 | −10.093±0.037 | 1.37 ± 0.19 × 105 |
| FSR 1758 | −1.50 | 0.90 | 226.8±1.6 | −2.881±0.026 | 2.519±0.025 | 4.91 ± 0.51 × 105 |
| NGC 6380 | −0.75 | 1.17 | −6.54±1.48 | −2.183±0.031 | −3.233±0.030 | 3.41 ± 0.05 × 105 |
| Ton 2 | −0.70 | 1.24 | −184.72±1.12 | −5.904±0.031 | −0.755±0.029 | 4.31 ± 0.91 × 104 |
| Terzan 9 | −1.05 | 1.76 | 29.31±2.96 | −2.121±0.052 | −7.763±0.049 | 1.37 ± 0.16 × 105 |
| Djorg 2 | −0.65 | 0.94 | −148.05±1.38 | 0.662±0.042 | −2.983±0.037 | 1.34 ± 0.24 × 105 |
| NGC 6540 | −1.35 | 0.66 | −17.98±0.84 | −3.702±0.032 | −2.791±0.032 | 5.62 ± 0.37 × 104 |
| NGC 6558 | −1.32 | 0.44 | −194.69±0.81 | −1.720±0.036 | −4.144±0.034 | 3.13 ± 0.10 × 104 |
| NGC 6569 | −0.76 | 0.53 | −49.83±0.50 | −4.125±0.028 | −7.354±0.028 | 2.29 ± 0.21 × 105 |
| NGC 6642 | −1.26 | 0.40 | −33.23±1.13 | −0.173±0.030 | −3.892±0.030 | 3.95 ± 0.13 × 104 |
| NGC 6656 | −1.70 | 0.34 | −147.76±0.30 | 9.851±0.023 | −5.617±0.023 | 4.70 ± 0.06 × 105 |
| NGC 6717 | −1.26 | 0.22 | 32.45±1.44 | −3.125±0.027 | −5.008±0.027 | 2.63 ± 0.19 × 104 |
Notes. [Fe/H] and E(B-V) are from H10 (except for FSR 1758, whose values are taken from Barba et al. 2019). Vr, proper motions and mass are from Baumgardt et al. (2019) and Vasiliev & Baumgardt (2021), respectively (except for FSR 1758, whose Vr is from Villanova et al. 2019).
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