\begin{table}%T1
\caption{\label{Table_2}Derived maximum velocities where the blue and red wings reach the continuum.
Listed are some forbidden emission lines and some Balmer lines in the FEROS spectrum whose
maximum wing velocities could be determined well and which are not blended.} 
%\centering
\par
\begin{tabular}{ccrr}
\hline
\hline
Ion & $\lambda$ &   $v_{\rm blue}$ & $v_{\rm red}$ \\
    &  [\AA] &  [km s$^{-1}$]  &  [km s$^{-1}$] \\
\hline
O{\sc iii}  & 4363 & --75 & +45 \\
O{\sc iii}  & 4959 & --80 & +65  \\
O{\sc iii}  & 5007 & --70 & +60 \\
O{\sc i}    & 5577 & --25 & +25 \\
O{\sc i}    & 6300 & --50 & +40 \\
O{\sc i}    & 6364 & --50 & +30 \\
S{\sc iii}  & 6312 & --60 & +50 \\
S{\sc ii}   & 4068 & --25 & +25 \\
S{\sc ii}   & 4076 & --50 & +35 \\
S{\sc ii}   & 6716 & --50 & +30 \\
S{\sc ii}   & 6731 & --50 & +35 \\
N{\sc ii}   & 5755 & --70 & +20 \\
N{\sc ii}   & 6548 & --70 & +45 \\
N{\sc ii}   & 6584 & --80 & +50 \\
Fe{\sc ii}  & 7155 & --40 & +30 \\
Cl{\sc iii} & 5517 & --30 & +100 \\
Cl{\sc iii} & 5538 & --50 & +40 \\
H$\alpha$   & 6563 & --1800 & +1800 \\
H$\beta$    & 4861 & --160 & +160 \\
H$\gamma$   & 4340 & --140 & +140 \\
H$\delta$   & 4101 & --100 & +100 \\
H$\epsilon$ & 3970 & --100 & +100 \\
H8          & 3889 & --100 & +40 \\
\hline
\end{tabular}
\end{table}