\begin{table}%t5
%\centering
\par
\caption {Summary of the parameters used to compute the spectrum in 2D geometry
using the \citet{bh05} code. Note that the density contrast between equator and pole is given by~$1+a$ for oblate models, and~$1/(1+a)$ for prolate models. 
\label{2dmodel}}
%\centering
\par
\begin{tabular}{c c c c c c c c}
\hline\hline
Model & Density  & $a$ & $b$ & Velocity & $VB1$ & $VB2$ & $VB3$ \\
& profile & & & changes? & & & \\
\hline								    %original model number
 1   & oblate	      & 1  & 2 & no	      &  \ldots  & \ldots  & \ldots   \\ %2 
 2   & prolate	      & 1  & 2 & no	      &  \ldots  & \ldots  & \ldots   \\ %16
 3   & oblate	      & 3  & 2 & no	      &  \ldots  & \ldots  & \ldots   \\ %3 
 4   & oblate	      & 3  & 5 & no	      &  \ldots  & \ldots  & \ldots   \\ %7 
 5   & oblate	      & 7  & 2 & no	      &  \ldots  & \ldots  & \ldots   \\ %6 
 6   & oblate	      & 7  & 5 & no	      &  \ldots  & \ldots  & \ldots   \\ %8 
 7   & oblate	      & 15 & 2 & no	      &  \ldots  & \ldots  & \ldots   \\ %9 
 8   & none	      & \ldots  & \ldots & yes        &  0.2 & 0.8 & 4    \\ %11   			      
 9   & oblate	      & 3  & 2 & yes	      &  0.8 & 2.2 & 4    \\ %23
\hline
\end{tabular}
\end{table}