Table 4: Observed and reddening-corrected emission line intensities, $F(\lambda )$ and $I(\lambda )$, respectively (normalized to H$\beta =100$). Positions A, B and C correspond to $\Delta \delta =0\hbox {$^{\prime \prime }$ }$, 8 $^{\prime \prime }$ N, and 7 $^{\prime \prime }$ S, respectively. The spectrum of ESO 370-9 was obtained at $\Delta \delta =44\hbox {$^{\prime \prime }$ }$ S.
\begin{displaymath}\begin{tabular}{l@{~~}r@{~}l@{~~~} r@{~~}r@{~~}r@{}c@{~~~~} ... ...& & & 0.91 & & & & 1.20 & & & & 1.53 \\ \hline \end{tabular} \end{displaymath}


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