\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}