\begin{table}%t5
\caption{\label{v945_pars}Probable V945~Cen model parameters and their formal
error estimates, where $\Omega$ is the value of the Roche-model potential used
in the WD program, and $L_i$ are the relative luminosities
of the components in individual photometric passbands.}
%\centerline
{\small
\begin{tabular}{lccccccc}
\hline
\hline\noalign{\smallskip}
&& \multicolumn{3}{c}{Solution in the absence of 3rd light:} &
\multicolumn{3}{c}{Solution in the presence of 3rd light:} \\
Parameter: &                & Primary &        & Secondary & Primary && Secondary \\
\noalign{\smallskip}\hline\noalign{\smallskip}
$a$                       &$(R_{\sun})$ && $5.86 \pm 0.21$ &
                                        && $5.63 \pm 0.18$ & \\
$i$                       &$({}^\circ)$ && $23.0^*$ &
                                        && $24.0^*$ & \\
$\Omega$                  &             & $3.625 \pm 0.018$ && $3.695 \pm 0.012$
                                        & $3.496 \pm 0.024$ && $3.608 \pm 0.015$ \\
$T_{\rm eff}$          &(K)          & $13000^*$  && $10930 \pm 40$
                                        & $13000^*$  && $10687 \pm 52$ \\
$M$                       &($M_{\sun}$) & $3.74 \pm 0.58$ && $2.67 \pm 0.54$
                                        & $3.32 \pm 0.51$ && $2.37 \pm 0.48$ \\
$R$                       &($R_{\sun}$) & $2.20 \pm 0.09$ && $1.73 \pm 0.07$
                                        & $2.09 \pm 0.12$ && $1.67 \pm 0.09$ \\
$L$                       &($L_{\sun}$) & $123  \pm 20$   && $35 \pm 6$
                                        & $111  \pm 21$   && $37 \pm 7$ \\
$M_{\rm bol}$          &(mag)        & $-0.50 \pm 0.2$ && $0.87 \pm 0.2$
                                        & $-0.38 \pm 0.2$  && $0.95 \pm 0.2$ \\
$\logg$                   &[cgs]        & $4.3 \pm 0.1$ && $4.4 \pm 0.1$
                                        & $4.3 \pm 0.1$ && $4.4 \pm 0.1$ \\
$L_i$ & $B$ band & 0.684 & & 0.316 & 0.534 & 0.227 & 0.239  \\
$L_i$ &$B1$ band & 0.688 & & 0.312 & 0.536 & 0.223 & 0.241  \\
$L_i$ &$B2$ band & 0.679 & & 0.321 & 0.530 & 0.232 & 0.238  \\
$L_i$ &$G$  band & 0.667 & & 0.333 & 0.517 & 0.242 & 0.242  \\
$L_i$ &$U$  band & 0.749 & & 0.251 & 0.620 & 0.184 & 0.197  \\
$L_i$ &$V$  band & 0.669 & & 0.331 & 0.519 & 0.240 & 0.241  \\
$L_i$ &$V1$ band & 0.670 & & 0.330 & 0.520 & 0.240 & 0.240  \\
$L_i$ &$H$p band & 0.679 & & 0.321 & 0.529 & 0.232 & 0.239  \\
\hline
\end{tabular}}
\tablefoot{They are normalized in
such a way that $L_1+L_2=1$ for the first model without the third light,
and $L_1+L_2+L_3=1$ for the triple-star model. Note that for this model,
the values of $L_3$ are tabulated in the central column between
the primary and secondary.\\
$^*$~Values denoted with an asterisk are \emph{fixed}.}
\end{table}