\begin{table}%T2
\caption{Stellar parameters obtained from the fits for different
cases. Case A is obtained ignoring veiling effects and gravitational darkening;
Case~B is obtained by accounting only for the veiling effects; for Cases~C, D,
and~E, veiling effects and gravitational darkening are taken into account with
a relative angular speed of the star at 80, 90, and 95\%, respectively, of its
break-up velocity (see Sect.~\ref{param}).}
\label{cases}
%\centering
\par
\begin{tabular}{llll}
\cline{1-3}\\[-3mm]
\cline{1-3}
Case			   & A               & B               \\ 
\cline{1-3}
$T_{\rm eff}$ (kK)	   & 17.5 $\pm$ 1    & 19.1 $\pm$ 1    \\
$\log~g$ (cgs)	           & 3.30 $\pm$ 0.10 & 3.91 $\pm$ 0.10 \\
$v\sin~i$ (km~s$^{-1}$)   & 176 $\pm$ 5     & 167 $\pm$ 5     \\
\hline
Case			      & C               & D               & E               \\
\hline
$\Omega \over \Omega_{\rm c}$ & 0.80            & 0.90            & 0.95            \\
$T_{\rm eff}$ (kK)	      & 19.6 $\pm$ 1.5  & 19.8 $\pm$ 1.5  & 20.2 $\pm$ 1.5  \\
$\log~g$ (cgs)	              & 4.04 $\pm$ 0.15 & 4.08 $\pm$ 0.15 & 4.11 $\pm$ 0.15 \\
$v\sin~i$ (km~s$^{-1}$)      & 170 $\pm$ 10    & 173 $\pm$ 10    & 177 $\pm$ 10    \\
$V_{\rm eq}$ (km~s$^{-1}$)   & 312 $\pm$ 20    & 381 $\pm$ 25    & 453 $\pm$ 24    \\
$i$ ($^{\circ}$)              & 33 $\pm$ 3      & 27 $\pm$ 2      & 23 $\pm$ 2      \\
$T_{\rm pol}$ (kK)	      & 20.6 $\pm$ 1.3  & 21.3 $\pm$ 1.4  & 22.2 $\pm$ 1.3  \\
$\log~g_{\rm pol}$ (cgs)	      & 4.08 $\pm$ 0.12 & 4.13 $\pm$ 0.12 & 4.17 $\pm$ 0.12 \\
$R_{\rm pol}$ ($R_\odot$)     & 3.93 $\pm$ 0.70 & 3.67 $\pm$ 0.66 & 3.55 $\pm$ 0.64 \\
$R_{\rm eq}$ ($R_\odot$)      & 4.62 $\pm$ 0.83 & 4.68 $\pm$ 0.83 & 4.80 $\pm$ 0.87 \\
$M$ ($M_\odot$)                 & 6.81 $\pm$ 0.81 & 6.81 $\pm$ 0.80 & 6.97 $\pm$ 0.85 \\
$L$ ($L_\odot$)                 & 3.35 $\pm$ 0.21 & 3.32 $\pm$ 0.21 & 3.34 $\pm$ 0.22 \\
$f_{\rm rot}$ (c~d$^{-1}$)   & 1.35 $\pm$ 0.35 & 1.63 $\pm$ 0.40 & 1.88 $\pm$ 0.46 \\
dist (pc)	              & 205 $\pm$ 70    & 228 $\pm$ 80    & 248 $\pm$ 85    \\
\hline
\end{tabular} 
\end{table}