Table 8: The physical parameters of the component stars of $\beta $ Aur derived from the JKTEBOP analysis and the circular spectroscopic orbit of Smith (1948). The effective temperatures are from NJ94.
\begin{displaymath}{ \begin{tabular}{l r@{~$\pm$~}l r@{~$\pm$~}l} \hline \hline ... ... $*$ & 0.448 & 0.094 & 0.676 & 0.095 \\ \hline \end{tabular}} \end{displaymath}
* Calculated assuming $\ensuremath{L_\odot} = 3.826 \times 10^{26}$ W
and $\ensuremath{M_{\rm bol}}\hbox{$\odot$ }= 4.75$ (Zombeck 1990).

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