\begin{table}%T3
\par
%\centering
\par
\caption{Parameters of the binary orbit for the SB2 star HD~62454.
Our data together with those of Kaye et al. (1999) lead to a final rms of the 
residuals of 1.81~\kms.
}
\label{table2}$$
\begin{tabular}{rcl}
\hline\hline
$P$            & = & $11.61550 \pm 0.00015$~d    \\
$T_0$          & = & $2450996.55 \pm 0.04$~d  \\
$e$            & = & $0.205 \pm 0.005$           \\
$\gamma$       & = & $7.5 \pm 0.2$~\kms \\
$K_1$          & = & $49.4 \pm 0.4$~\kms \\
$\omega_1$     & = & $261.0 \pm 1.3^{\circ}$     \\
$K_2$          & = & $66.0 \pm 0.4$~\kms \\
$\omega_2$     & = & $81.0 \pm 1.3^{\circ}$     \\
$a_1 \sin i$   & = & $(7.73 \pm 0.07)\times10^6$~km   \\
$M_1.\sin^3 i$ & = & $0.994 \pm 0.013$~$M_{\sun}$ \\
$a_2 \sin i$   & = & $(10.31 \pm 0.08)\times10^6$~km   \\
$M_2.\sin^3 i$ & = & $0.745 \pm 0.011$~$M_{\sun}$ \\
\hline
\end{tabular}$$
\end{table}