Table 5: Comparison between the measured LD coefficients for $\beta $ Aur and predictions calculated using theoretical model atmospheres. Bilinear interpolation was used to interpolate the tabulated theoretical coefficients to the effective temperatures and surface gravities for $\beta $ Aur given by NJ94. A solar metal abundance and a microturbulence velocity of 2 km s-1 have been adopted and results are quoted for the Johnson V and Cousins R bandpasses.
\begin{displaymath}\begin{tabular}{l c r@{~$\pm$~}l rr rr rr rr rr } \hline \hli...
... 0.344 & 0.400 & 0.374 & 0.340 & 0.294 \\
\hline \end{tabular}\end{displaymath}
References: Van Hamme is Van Hamme (1993); Díaz-Cordoves is Díaz-Cordovés et al. (1995) and Claret et al. (1995);
Claret is Claret (2000a) and Claret & Hauschildt is Claret & Hauschildt (2003).

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