Table 5
Distance modulus ((m–M)0), extinction (Av), ages, and the Li-rich limit estimation (A(Li)max).
| Cluster | (m−M)0 | AV | Age (Ga) | A(Li)max (dex) |
|---|---|---|---|---|
| IC2714 | 10.64 | 0.99 | 0.47 | 1.46 |
| IC4651 | 9.96 | 0.41 | 1.58 | 1.46 |
| IC4756 | 8.40 | 0.40 | 0.98 | 1.26 |
| NGC1662 | 7.84 | 0.62 | 0.91 | 1.46 |
| NGC2204 | 13.01 | 0.01 | 2.09 | 1.37 |
| NGC2251 | 10.71 | 0.72 | 0.31 | 1.46 |
| NGC2287 | 9.24 | 0.06 | 0.20 | 1.26 |
| NGC2345 | 12.32 | 1.91 | 0.07 | 1.37 |
| NGC2354 | 10.62 | 0.38 | 1.66 | 1.26 |
| NGC2360 | 10.24 | 0.11 | 1.12 | 1.26 |
| NGC2423 | 9.84 | 0.29 | 1.02 | 1.46 |
| NGC2447 | 10.09 | 0.11 | 0.56 | 1.26 |
| NGC2477 | 10.88 | 0.95 | 0.83 | 1.45 |
| NGC2506 | 12.54 | 0.17 | 2.14 | 1.37 |
| NGC2539 | 10.52 | 0.21 | 0.68 | 1.46 |
| NGC2567 | 11.35 | 0.47 | 0.34 | 1.46 |
| NGC2682 | 9.73 | 0.12 | 3.63 | 1.46 |
| NGC2925 | 9.38 | 0.29 | 0.15 | 1.46 |
| NGC2972 | 11.49 | 1.20 | 0.49 | 1.45 |
| NGC3114 | 10.11 | 0.26 | 0.13 | 1.46 |
| NGC3532 | 8.39 | 0.07 | 0.35 | 1.40(†) |
| NGC3680 | 10.15 | 0.20 | 1.78 | 1.26 |
| NGC4349 | 11.29 | 1.16 | 0.32 | 1.26 |
| NGC5822 | 9.72 | 0.35 | 0.89 | 1.46 |
| NGC6067 | 11.51 | 0.88 | 0.13 | 1.53(†) |
| NGC6134 | 10.36 | 0.87 | 1.45 | 1.45 |
| NGC6208 | 10.34 | 0.63 | 1.74 | 1.26 |
| NGC6281 | 8.63 | 0.42 | 0.32 | 1.46 |
| NGC6425 | 10.04 | 0.69 | 0.54 | 1.46 |
| NGC6494 | 9.35 | 0.85 | 0.38 | 1.46 |
| NGC6633 | 7.87 | 0.45 | 0.78 | 1.46 |
| NGC6705 | 11.84 | 1.10 | 0.22 | 1.54(†) |
Notes. The ages, distance modulus, and extinction are derived based on the methodology of Bossini et al. (2019) and the A(Li)max is an estimation on the maximum Li abundance estimated from Randich et al. (2020) and Romano et al. (2021).(†) These values are taken directly from Randich et al. (2020) and Romano et al. (2021), (or their average), while the rest are estimations depending on the OC metallicity of this work.
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