\begin{table}%t1
        \caption {\label{tab1}Stellar parameters of HD 110014.   }
                                       %\centerline
 {
                                \begin{tabular}{p{0.35\linewidth}p{0.25\linewidth}l}
                                        \hline \hline
                                        Spectral type & K2III&\\
                                        $V$& 4.66&mag\\
                                        $M_v$ &$-0.11 \pm 0.06$&mag\\
                                        $(B-V)$& 1.24&mag\\
                                        Parallax& 11.11 $\pm$ 0.29&mas\\
                                        Distance& 90.0 $\pm$ 2.3&pc\\
                                        \Teff &4445 $\pm$ 70&K\\
                                        \feh& 0.19 $\pm$ 0.05&\\
                                         Age& $0.95 \pm 0.40$&Gyr \\
                                        $M$ &$2.17 \pm 0.28$&\Msun \\
                                        Log {$g$}& $2.10 \pm 0.10$&c.g.s.\\
                                        $R$& $20.9 \pm 1.1$&\Rsun\\
                                        $E(b-v)$& $0.05 \pm 0.04$&mag\\
                                        $\theta$& $2.16 \pm 0.13$&mas\\
                                        \Vsini& 2.0&km~s$^{-1}$\\
                                        $P_{\rm rot}/\sin i$ &513&day\\
                                                \hline
                \end{tabular}}
                \smallskip
                The stellar parameters were
originally computed 
        by da Silva et~al. (\cite{daSilva06}). Log~($g$), Mass, Radius and  age have been
re-computed in the present paper after adopting the new Hipparcos parallaxes
(van~Leeuwen \cite{vanLeeuwen07}).
\end{table}