\begin{table} %tab1
\caption{Fluxes of the \oiii\ emission for  the brightest areas of the
P~Cygni GL.}
\label{fluxes}
%\begin{flushleft}
%\centerline
{
\begin{tabular}{lllllll}
\hline
\hline
\noalign{\smallskip}
\bf Eastern complex & 3$\arcmin$ & 4$\arcmin$ & 6$\arcmin$ & 8$\arcmin$ &
10$\arcmin$ & 12$\arcmin$ \\
\hline
North  & 2.25 & 2.71 & 2.01 & 2.23 & 2.10 & 2.17 \\
South  &  & 1.91 &  & 1.85 &  & \\
\hline
\hline
\bf Western complex & 3$\arcmin$ & 3$\arcmin$.5 & 4$\arcmin$ & 4$\arcmin$.5
& 6$\arcmin$.5 &  \\
\hline
North & 2.41 & 2.17 & 2.73 & & & \\
North--west & 2.73 & &  & 1.95 & 3.76 \\
South--west & & & 2.30 & & \\
\hline
\end{tabular}}
\smallskip
%\end{flushleft}
${\rm }$ All arcmin values are away from P Cygni. \\
${\rm }$ Fluxes in units of $10^{-16}$ erg s$^{-1}$ cm$^{-2}$
arcsec$^{-2}$. \\
$^{\rm}$ Median values over a 55\arcsec~$\times$~55\arcsec\ box. \\
$^{\rm}$ Fluxes are uncorrected for interstellar extinction.
\end{table}