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Table 2
Effects on derived abundances resulting from model changes for the star HD 52711.
| Ion | ΔTeff + 100 K | Δlog g + 0.3 | Δvt + 0.3 km s-1 | Total |
|
|
||||
| [O i] | 0.03 | 0.13 | 0.01 | 0.13 |
| Na i | 0.05 | −0.02 | −0.01 | 0.05 |
| Mg i | 0.05 | −0.02 | −0.03 | 0.06 |
| Al i | 0.04 | 0.00 | 0.00 | 0.04 |
| Si i | 0.03 | 0.01 | −0.01 | 0.03 |
| Ca i | 0.07 | −0.01 | −0.02 | 0.07 |
| Sc ii | −0.00 | 0.11 | −0.04 | 0.12 |
| Ti i | 0.09 | 0.00 | −0.01 | 0.09 |
| Ti ii | 0.01 | 0.12 | −0.05 | 0.13 |
| V i | 0.11 | −0.00 | −0.01 | 0.11 |
| Cr i | 0.08 | −0.02 | −0.06 | 0.10 |
| Cr ii | −0.03 | 0.10 | −0.09 | 0.14 |
| Fe i | 0.07 | −0.02 | −0.07 | 0.10 |
| Fe ii | −0.02 | 0.11 | −0.07 | 0.13 |
| Co i | 0.08 | 0.01 | −0.01 | 0.08 |
| Ni i | 0.06 | −0.00 | −0.04 | 0.07 |
| Y ii | 0.02 | 0.10 | −0.12 | 0.16 |
| Zr i | 0.11 | 0.01 | 0.01 | 0.11 |
| Zr ii | 0.02 | 0.13 | 0.01 | 0.13 |
| Ba ii | 0.06 | 0.08 | −0.18 | 0.21 |
| La ii | 0.03 | 0.12 | 0.01 | 0.12 |
| Ce ii | 0.03 | 0.11 | 0.01 | 0.11 |
| Pr ii | 0.02 | 0.12 | 0.01 | 0.12 |
| Nd ii | 0.03 | 0.12 | −0.01 | 0.12 |
| Sm ii | 0.04 | 0.11 | −0.01 | 0.12 |
| Eu ii | 0.03 | 0.12 | 0.01 | 0.12 |
Notes. The table entries show the effects on the logarithmic abundances relative to hydrogen, Δ [El/H].
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