Beryllium abundances and star formation in the halo and in the thick disk

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Table 8:

The uncertainties of the Li abundances, calculated in this work, introduced by the uncertainties of the atmospheric parameters.
Star	$\sigma_{\rm T_{eff}}$	$\sigma_{\log~ g}$	$\sigma_{\rm\xi}$	$\sigma_{\rm [Fe/H]}$	$\sigma_{\rm cont.}$	$\sigma_{\rm total}$
HIP 74067	$\pm$ 0.10	$\pm$ 0.00	$\pm$ 0.00	$\pm$ 0.00	$\pm$ 0.05	$\pm$ 0.11

The total uncertainty also includes the effect of the continuum
uncertainties ( $\pm$ 0.05 dex) on the Li abundance.

Source LaTeX | All tables | In the text

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