\begin{table}
\caption{Stellar parameters used to model the line-profile
variations using the spectral-synthesis codes {\sc bruce} and {\sc
kylie} \citep{Bruce}.} \label{tbl:modeling_parameters}
%\centerline
{
\begin{tabular}{ll} \hline\hline Parameter & Value \\
\hline
Equatorial rotational velocity (km~s$^{-1}$) & 75 \\
Inclination angle ($^\circ$) & 80.67 \\
Polar radius ($R_\odot$) & 0.15 \\
Polar temperature (K) & 31~300 \\
Polar gravity (cm~s$^{-2}$) & 5.77 \\
Pulsation period$^{a}$ (s) & 183.98\\
\hline
\end{tabular}}
{$^{a}$~The period detected in our VLT/{\sc uves} data set and in
all photometric campaigns on \nyvir\ (see Paper I).}
\end{table}