Table 1
Limits over which a star can be considered lithium rich for every cluster in our sample (A(Li)max (dex)).
| Cluster | A(Li)max (dex) | [Fe/H] (dex) |
|---|---|---|
| IC4651 | 1.46 | −0.01 |
| IC4756 | 1.26 | −0.12 |
| NGC2345 | 1.37 | −0.22 |
| NGC2423 | 1.46 | −0.03 |
| NGC3114 | 1.46 | −0.10 |
| NGC3532 | 1.40 | −0.08 |
| NGC3680 | 1.26 | −0.15 |
| NGC4349 | 1.26 | −0.11 |
| NGC5822 | 1.46 | −0.10 |
| NGC6705 | 1.54(1) | 0.07 |
Notes. Also included is the metallicity of each cluster ([Fe/H]). The note (1) indicates A(Li)max was derived in Randich et al. (2020); Romano et al. (2021). The remainder of these limits and metallicities were derived in Tsantaki et al. (2023).
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