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Table 4
Effect introduced in the Be abundance by the uncertainties of each of the atmospheric parameters and by the uncertainty of the fitting itself related to the level of the continuum and the S/N.
| Star | σTeff | σlog g | σξ | σ [Fe/H] | σfitt. | σtotal |
|
|
||||||
| SHJM2 | ± 0.05 | ± 0.10 | ± 0.00 | ± 0.03 | ± 0.05 | ± 0.13 |
| R14 | ± 0.05 | ± 0.10 | ± 0.05 | ± 0.00 | ± 0.10 | ± 0.16 |
| VXR67 | ± 0.10 | ± 0.20 | ± 0.10 | ± 0.00 | ± 0.20 | ± 0.32 |
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