\begin{table}%t3
\caption{\label{tbl:cenpeak}Properties of the central emission peaks.}
%\centerline
{\small
\begin{tabular}{lcccclc}
\hline 
\hline 
UGC            & NGC & Classn. & Dist. & Peak & Res & {\it FWHM}\\
               &     &         & Mpc &       &          & kpc\\
\hline 
3685           &  --  &    SB(rs)b    & 26 & Y & U    & $<$0.17 \\ 
4273           & 2543 &    SB(s)b     & 35 & Y & R    &    0.65 \\ 
4484           & 2608 &    SB(s)b     & 32 & Y & R    &    0.34 \\ 
4574           & 2633 &    SB(s)b     & 31 & Y & R    &    0.62 \\ 
4705$^1$  & 2710 &    SB(rs)b    & 36 & Y & R$+$ &    1.10 \\
4708           & 2712 &    SB(r)b:    & 29 & Y & R$+$ &    1.20 \\ 
6077           & 3485 &    SB(r)b:    & 27 & Y & R    &    0.29 \\ 
6123$^2$  & 3507 &    SB(s)b     & 21 & Y & R?   &     --  \\ 
6595$^3$  & 3769 &    SB(r)b:    & 12 & Y & R$+$ &    0.32 \\ 
7002           & 4037 &    SB(rs)b:   & 18 & Y & R?   &    0.24 \\ 
7523$^4$  & 4394 & (R)SB(r)b:    & 18 & Y & R$+$ &    0.46 \\ 
7753$^5$  & 4548 &    SB(rs)b    & 18 & Y & R$+$ &    0.45 \\ 
9649$^6$  & 5832 &    SB(rs)b?   &  8 & N & --   &     --  \\ 
12699$^7$ & 7714 &    SB(s)b:p   & 31 & Y & R?   &    0.32 \\ 
\hline 
\end{tabular}}
\par
\medskip
$^1$~Emission elongated along bar axis. $^2$~LINER; foreground star contamination, so not in mean profiles. $^3$~Interacting with NGC~3769A, type Sm. $^4$~LINER; Smooth extended emission, possible ENER. $^5$~M91; LINER/Seyfert; possible ENER. $^6$~Classified as SBc in UGC. $^7$~\HII/LINER; tidally distorted.\\
 For each galaxy, we
list the UGC and NGC catalogue numbers, the full galaxy classifications from 
\citet{deva91}, the distance in Mpc from Paper~I, whether or not the 
galaxy exhibits a central peak in \Ha\ emission, the resolution of the 
peak as explained
in Sect. \ref{sec:cen_peak}, and the FWHM of the emission, in kpc.
All LINER/Seyfert classifications in the footnotes are taken from
the NASA/IPAC Extragalactic Database (NED).
\end{table}