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Table 6.
Li depletion boundary (LDB) in open clusters older than 20 Myr, ordered by increasing distance.
| Name | d | SpT | Age (LDB) | Age (Other) | Mass | Ref. |
|---|---|---|---|---|---|---|
| pc | Li | Myr | Myr | M⊙ | ||
| Hyades | 47 | L4 | 650 ± 70 | 570–900 | 0.065 | Martín et al. (2018) |
| Coma Ber | 87 | > L2.5 | > 550 | 300–1000 | < 0.07 | This work |
| Pleiades | 130 | M6.5 | 112 ± 5 | 70–160 | 0.075 | Dahm (2015) |
| IC 2391 | 146 | M5 | 50 ± 5 | 30–75 | 0.12 | Barrado y Navascués et al. (2004) |
| IC 2602 | 152 | M5.5 | 46 ± 6 | 25–70 | 0.12 | Dobbie et al. (2010) |
| Alpha Per | 190 | M6.5 | 85 ± 10 | 50–70 | 0.08 | Barrado y Navascués et al. (2004) |
| Blanco 1 | 207 | M7 | 126 ± 14 | 150–500 | 0.072 | Juarez et al. (2014) |
| IC 4665 | 385 | M4 | 28 ± 5 | 30–100 | 0.24 | Manzi et al. (2008) |
| NGC 2547 | 430 | M4 | 35 ± 4 | 20–80 | 0.17 | Jeffries & Oliveira (2005) |
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