... sample[*]
Based on observations collected at the European Southern Observatory, Chile, using FEROS spectrograph (proposals ID: 69.D-0338-70.D-0081).
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...[*]
Table 3 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/454/581
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...[*]
Tables 2, 5, 6, 8-10 are only available in electronic form at http://www.edpsciences.org
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... than 1.0)[*]
Two pairs with larger magnitude difference, HIP 76446 and HIP 78024, were also observed and included in this work.
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... star[*]
The slopes actually have a small dependence on effective temperature, but the impact of this on our results is negligible because of the use of an iterative procedure until convergence.
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... difference[*]
The epoch of the observation of Fuhrmann (2004) is not reported in his paper.
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... turbulence[*]
The parameterization of turbulence used in the quoted models was fixed to minimize the surface lithium abundance changes in Population II stars.
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Copyright ESO 2006