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Table 4
Uncertainties in the non-LTE analysis of Fe i and Fe ii in selected stars.
| Changes in non-LTE abundances, [Fe/H], with regard | ||||||||
| to those in Col. 10 (SH = 0.1) of Table 3 | ||||||||
|
|
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| Input parameter | HD 61421 | HD 84937 | HD 122563 | |||||
| Fe i | Fe ii | Fe i | Fe ii | Fe i | Fe ii | |||
|
|
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| H i collisions: | ||||||||
| SH = 0 | −0.02 | 0.01 | +0.04 | +0.02 | +0.19 | +0.11 | ||
| SH = 1 | −0.03 | 0.01 | −0.13 | 0.00 | −0.13 | 0.00 | ||
| SH = 2 | −0.03 | 0.00 | −0.14 | 0.00 | −0.15 | 0.00 | ||
| SH = 0.1/0 for | 0.00 | 0.00 | +0.06 | 0.00 | +0.08 | +0.03 | ||
| allowed/forbidden transitions | ||||||||
| Reduced model atom, SH = 0.1 | +0.01 | +0.01 | +0.02 | +0.01 | +0.07 | 0.00 | ||
| Stellar parameters: | ||||||||
| ΔTeff = −80 K | – | – | – | – | −0.14 | +0.01 | ||
| ΔTeff = +80 K | +0.06 | 0.00 | +0.06 | +0.03 | – | – | ||
| Δlog g = −0.1 | – | – | 0.00 | −0.03 | +0.02 | −0.04 | ||
| ΔVmic = −0.1 km s-1 | 0.02 | 0.04 | 0.00 | 0.01 | 0.02 | 0.01 | ||
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