Table C.1.
Tc and Li abundances of the sample stars as well as of the stars from S18, S19, and S20.
| Star | log ϵTc | log ϵLi | [Li/Fe] |
|---|---|---|---|
| HR Peg | −1.3 | 1.3 | 0.6 |
| HD 28833 | −1.2 | < −0.3 | < −1.05 |
| V812 Oph | 1.0 | – | – |
| AA Cam | −0.4 | < −0.3 | < −1.02 |
| V1139 Tau | −0.6 | – | – |
| KR CMa | – | – | – |
| CSS 151 | −0.1 | < −0.6 | < −1.4 |
| CD −27°5131 | – | – | – |
| BD −18°2608 | −0.1 | < 0.4 | < −0.34 |
| V679 Oph | 0.5 | 0.0 | −0.53 |
| CSS 454 | 0.5 | < −0.6 | < −1.26 |
| CSS 1152 | 0.5 | 0.0 | −0.91 |
| HD 64147 | −0.1 | < −0.6 | < −0.98 |
| o1 Ori | −0.4 | < −0.6 | < −1.37 |
| BD +79°156 | −0.7 | < 0.1 | < −0.78 |
| V915 Aql | −0.2 | < −0.6 | < −1.15 |
| UY Cen | – | −0.3 | −1.35 |
| NQ Pup | −0.3 | < −0.6 | < −1.35 |
| HD 357941 | −0.6 | < −0.2 | < −0.77 |
| CSS 154 | −0.6 | < −0.3 | < −1.06 |
| CSS 182 | 0.0 | < −0.6 | < −1.25 |
| CD −29°5912 | −0.6 | < −0.9 | < −1.55 |
| BD +34°1698 | −0.6 | < −0.2 | −0.55 |
Notes. A dash indicates that the agreement between the observed and the synthetic spectra was too poor and that the (unique) line usually providing the abundance for the considered element had to be rejected. The “< ” symbol is used when the line is still usable but only provides an upper limit on the abundance.
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