Table 3
Average for log ϵ(X) and [X/Fe].
| Star | El | log ϵ(X) | [X/Fe] | σ l | σ f |
|
|
|||||
| HD 9362* | Li | –0.34 | ... | 0.14 | 0.16 |
| HD 9362* | C | 8.19 | 0.01 | 0.10 | 0.10 |
| HD 9362* | N | 7.73 | 0.15 | 0.09 | 0.08 |
| HD 9362* | O | 8.54 | 0.14 | 0.17 | 0.17 |
| HD 9362* | Mn | 4.80 | -0.25 | 0.11 | 0.10 |
| HD 9362* | Cu | 3.66 | -0.21 | 0.12 | 0.11 |
| HD 9362* | Zn | 4.01 | -0.25 | 0.13 | 0.13 |
Notes. Uncertainties on log ϵ(X) and [X/Fe] are represented by σl, and σf, respectively. Given that Smiljanic et al. (2007) used HD 113226 as a reference star, there is no uncertainty designed to it. The full table is only available at the CDS. The symbol “*” indicates those stars that were considered to be normal instead of barium stars by Smiljanic et al. (2007). From the line 351, the data of Allen & Barbuy (2006a) with corrected uncertainties are shown. From the line 1001, the solar abundances and their references are shown.
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