Table 2.
Li abundances for the 714 stars†.
| HIP | Teff | ∈Teff | log g | ∈ log g | [Fe/H] | ∈[Fe/H] | M | Mhigh | Mlow | Age | Agehigh | Agelow | A(Li)NLTE |
|
|
ΔNLTE | Flag |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
| 1931 | 5990 | 58 | 4.45 | 0.08 | 0.34 | 0.07 | 1.16 | 1.15 | 1.21 | 1.5 | 0.7 | 2.7 | 2.43 | 2.38 | 2.48 | 0.04 | 0 |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
Notes.
For each star we give effective temperature, surface gravity, and metallicity and their estimated uncertainties. For the masses and ages, we give the best value and the the lower and upper estimates. These values are taken from Bensby et al. (2014). We then give the NLTE corrected A(Li) abundance and the low and high values determined by changing the effective temperature by its uncertainty. The Li NLTE corrections that were added are also given. The last column is a flag where the value “0” indicates a value from a well-fitted line. A value of “1” means that the Li abundance is an upper limit. The table is only available at the CDS.
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