Beryllium abundances along the evolutionary sequence of the open cluster IC 4651 – A new test for hydrodynamical stellar models

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Table 3:

The uncertainties of the Be abundance introduced by the uncertainties of the atmospheric parameters and by uncertainty of the fitting itself related to the level of the continuum and the S/N.
Star	$\sigma_{{T}_{\rm eff}}$	$\sigma_{\rm log{\it g}}$	$\sigma_{\rm\xi}$	$\sigma_{\rm [Fe/H]}$	$\sigma_{\rm fitt.}$	$\sigma_{\rm total}$
E 7	$\pm$ 0.03	$\pm$ 0.10	$\pm$ 0.00	$\pm$ 0.00	$\pm$ 0.05	$\pm$ 0.12
E 86	$\pm$ 0.05	$\pm$ 0.10	$\pm$ 0.05	$\pm$ 0.05	$\pm$ 0.10	$\pm$ 0.17
E 60	$\pm$ 0.15	$\pm$ 0.05	$\pm$ 0.03	$\pm$ 0.05	$\pm$ 0.20	$\pm$ 0.26

Source LaTeX | All tables | In the text

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