\begin{table}%t1
%\centering
\par
  \caption{\label{tab:Coefficients} Parameters of the calculated models,
    $a$ and $b$ are parameters used in Eq.~(\ref{eq:Polynomial}) with values of 
    gravity darkening $\beta$ according to \cite{Claret98}. Note that
    for all models profiles with $\beta = 0.0, 0.08$ and $0.25$ were analyzed.}
  \begin{tabular}{crrccc}
    \hline
    \hline
    \noalign{\smallskip}
    Model & $T_{\rm eff}^{\rm Pole}$ & $M/M_\odot$ & $\beta$ & $a$ & $b$\\
    \noalign{\smallskip}
    \hline
    \noalign{\smallskip}
    B0 & 30~000 & 17.5 & 0.25 & .740E--4 & --.345E--6\\
    A0 & 10~000 & 2.4 & 0.25 & .190E--3 & --.136E--5\\
    F0 &  7000 & 1.6 & 0.08 & .172E--3 & --.993E--6\\
    G0 &  5700 & 1.0 & 0.08 & .184E--3 & --.116E--5\\
    \hline
  \end{tabular}
\end{table}