\begin{table}%t2
\caption{Summary of the parameters of the nuclear bar as derived from the best fits to the 2MASS star count data.}\label{tab:res-Bdb}
%\centerline
 {\small \begin{tabular}{lllllll}
\hline\hline\noalign{\smallskip}
 $x_0^b$ & $y_0^b$ & $z_0^b$ &$\rho_0^b$ & $\alpha^b $ & $x_1$ &   $\chi^2$ \\
  kpc     & kpc      &   kpc   &              & deg        & kpc      &           \\
\hline
 0.141--0.150& 0.130--0.138& 0.095--0.097 & 0.141--0.150 & 60--120 &  0.0        & 0.357--0.376\\
 0.158--0.166& 0.115--0.133& 0.088--0.094 & 0.151--0.178 & 60--120 & 0.022--0.025& 0.331--0.346 \\
\hline                  
\end{tabular} }
\medskip
The first row are fits with $x_1$ fixed to 0 and the second row corresponds to fits with free $x_1$ to allow for lopsidedness. The full set of results as a function of the orientation of the bulge ($\alpha^B$) are listed in Tables~\ref{tab:res-Bdb1} to~\ref{tab:res-Bdb4}.          
\end{table}