\begin{table}%t8
%Table8
%\centering
\par
\caption{\label{tab8}X-ray luminosities (erg~s$^{-1}$) 
from the shocked region as predicted
by the hydrodynamical simulations.}
\begin{tabular}{lcc}
\hline\hline
Abundance & Flux at & Flux at \\
En.\ range & Apastron & Periastron \\
\hline
Solar && \\
{[0.5--10.0 keV]} & $2.33 (\pm 0.13) \times 10^{34}$ &
$6.24 (\pm 0.92) \times 10^{34}$ \\
{[2.0--10.0 keV]} & $0.40 (\pm 0.02) \times 10^{34}$ &
$0.35 (\pm 0.07) \times 10^{34}$ \\
WN && \\ 
{[0.5--10.0 keV]} & $1.18 (\pm 0.09) \times 10^{35}$ &
$2.44 (\pm 0.31) \times 10^{35}$ \\
{[2.0--10.0 keV]} & $1.85 (\pm 0.12) \times 10^{34}$ &
$2.14 (\pm 0.25) \times 10^{34}$ \\
\hline
\end{tabular}
\end{table}