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Table 6
Stars illustrated in Fig. 7 as having a high metallicity and low lithium abundance.
| Identifier | AgePARAM (Ga) | AgeLit (Ga) | U (km s−1) | Candidates |
|---|---|---|---|---|
| HD 166745 | 8.2 + 1.6 | … | −7.61 | • |
| HD 190647 | 8.9 + 1.0 | 8.0 + 1.2 | −32.37 | • |
| HD 22177 | 8.2 + 1.6 | 8.1 + 1.4 | −8.89 | • |
| HD 30306 | 8.4 + 1.7 | 8.5 + 2.7 | 5.00 | … |
| HD 45350 | 8.1 + 1.5 | 9.2 + 1.6 | 16.65 | … |
| HD 64640 | 9.5 + 1.7 | … | −23.83 | • |
| HD 73526 | 8.1 + 1.8 | … | −78.91 | • |
| Kepler 46 | 10.5 + 1.2 | 11.8 | 258.74 | … |
| HD 102117 | … | 8.1 + 1.4 | 13.35 | … |
| HD 108874 | … | 12.3 + 1.0 | 44.91 | … |
| HD 115585 | … | 8.5 + 1.2 | −50.14 | • |
| HD 117207 | … | 8.4 + 1.6 | −33.40 | • |
| HD 134606 | … | 12.2 + 1.1 | −20.98 | • |
| HD 145675 | … | 12.3 + 0.9 | 23.35 | … |
| HD 46375 | … | 10.0 + 1.4 | 9.22 | … |
| HD 76909 | … | 8.4 + 1.7 | 24.72 | … |
Notes. Both age estimates, either from the PARAM code or from the literature, are presented. The last column lists objects that are good candidates for validating the scenario proposed by Guiglion et al. (2019).
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