Table C.5.
The heavy (hs) and light (ls) s-process indices of the sample stars.
| Star | [ls/Fe] | [hs/Fe] | [hs/ls] | σ[hs/ls] | [s/Fe] | σ[s/Fe] |
|---|---|---|---|---|---|---|
| HR Peg | 0.43 | 0.26 | −0.16 | 0.27 | 0.31 | 0.31 |
| HD 288833 | 0.53 | – | – | – | – | – |
| V812 Oph | – | 1.12 | – | – | – | – |
| AA Cam | 0.33 | 0.12 | −0.20 | 0.32 | 0.24 | 0.36 |
| V1139 Tau | – | – | – | – | – | – |
| KR CMa | – | 0.61 | – | – | – | – |
| CSS 151 | 0.58 | 0.34 | −0.24 | 0.38 | 0.48 | 0.42 |
| CD −27°5131 | 0.73 | 0.80 | 0.07 | 0.26 | 0.79 | 0.35 |
| BD −18°2608 | 0.64 | 0.73 | 0.09 | 0.26 | 0.63 | 0.29 |
| V679 Oph | 1.47 | 1.47 | −0.01 | 0.32 | 1.46 | 0.43 |
| CSS 454 | 0.82 | 1.04 | 0.22 | 0.21 | 0.88 | 0.27 |
| CSS 1152 | 1.32 | 1.26 | −0.05 | 0.20 | 1.23 | 0.27 |
| HD 64147 | 0.45 | 0.47 | 0.02 | 0.26 | 0.43 | 0.33 |
| o1 Ori | 0.16 | −0.02 | −0.19 | 0.30 | 0.01 | 0.36 |
| BD +79°156 | 0.80 | 0.72 | −0.08 | 0.21 | 0.73 | 0.27 |
| V915 Aql | 0.28 | 0.47 | 0.19 | 0.27 | 0.36 | 0.37 |
| UY Cen | 1.12 | 1.07 | −0.04 | 0.57 | 0.92 | 0.85 |
| NQ Pup | 0.44 | 0.46 | 0.02 | 0.40 | 0.40 | 0.46 |
| HD 357941 | 0.21 | – | – | – | 0.24 | 0.75 |
| CSS 154 | 0.44 | – | – | – | 0.40 | 0.87 |
| CSS 182 | 0.63 | 0.70 | 0.07 | 0.62 | 0.66 | 0.82 |
| CD −29°5912 | 0.66 | 0.82 | 0.17 | 0.56 | 0.67 | 0.75 |
| BD +34°1698 | 0.80 | 0.9 | 0.09 | 0.40 | 0.87 | 0.59 |
Notes. The [ls/Fe] index has been derived using Y and Zr, whereas the [hs/Fe] index relies on Ba and Nd abundances. The error on the [hs/ls] ratio was computed by quadratically adding the error on the individual abundances of the elements considered to compute the [hs/Fe] and [ls/Fe] ratios. The same method is used to estimate the error on the [s/Fe] ratio, which is based on the abundances of Y, Zr, and Ba.
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