\begin{table}%t5
%\centering
\par
\caption{\label{tab5}All galaxies from which we obtained $V_{\rm max}$. 
In the case of \mseins\ A12~$=$~B8.
For an identification see finding charts in Fig.~\ref{fig3}.
In some cases there was no [OII] line within the spectra and we used other emission lines.}
\begin{tabular}{cccccccccc}
\hline\hline
Cluster &ID     &mem    &Type  &Incl. &$\delta$ &$r_{\rm d}$  &$V_{\rm max}$  &{\it EW} ([OII])      &$M_{B}$ \\
        &       &       &      &[deg] &[deg]    &[$''$]     &[km~s$^{-1}$]     &[\AA ]          &[mag] \\
(1)     & (2)   & (3)   &(4)   & (5)  & (6)     & (7)     & (8)       &(9)      & (10)  \\  
\hline
\mseins &A8     &yes    &+8 &45  &   5     &0.40     & 70~$\pm$~30 &72.8   &$-$20.19  \\
\mseins &A12    &yes    &+5 &50  &  43     &0.70     &220~$\pm$~59 &	  &$-$20.69   \\
\mseins &A15    &yes    &+5 &20  &  20     &0.57     &270~$\pm$~126&	  &$-$21.24   \\
\mseins &B1     &yes    &+5 &60  &  $-9$     &1.35     &130~$\pm$~23 &	  &$-$20.15   \\
\mseins &B3     &no     &+1 &55  &  63     &0.40     &320~$\pm$~129&5.1    &$-$21.26   \\
\mseins &B5     &yes    &+5 &60  &  10     &0.60     &150~$\pm$~26 &	  &$-$20.32   \\
\mseins &B8     &yes    &+5 &50  & $-17$     &0.70     &240~$\pm$~49 &	  &$-$20.69   \\
\mseins &B12    &yes    &+5 &50  &   8     &0.60     &160~$\pm$~32 &	  &$-$20.52   \\
\mseins &B14    &yes    &+5 &52  & $-50$     &1.02     &230~$\pm$~68 &15.7    &$-$21.48   \\
\hline 
\cldrei &B4     &yes    &+3 &20  & $-30$     &0.80     &400~$\pm$~135&5.1    &$-$22.13     \\
\cldrei &B7     &no     &+5 &35  &  25     &0.72     &320~$\pm$~62 &19.4   &$-$21.98     \\
\hline 
\clvier &A7     &no  	&+3 &54  & 19	   &0.45     &200~$\pm$~26 &12.3   &$-$20.94  \\
\clvier &A8     &yes 	&+8 &65  &$-$20	   &0.60     &150~$\pm$~18 &39.5   &$-$20.12  \\
\clvier &A11    &no  	&+3 &33  &  0	   &0.85     &350~$\pm$~96 &10.3   &$-$21.65  \\
\clvier &A13    &no  	&+5 &50  & 25	   &0.55     &202~$\pm$~29 &14.1   &$-$21.16  \\
\clvier &A18    &no  	&+5 &60  & 20	   &0.80     &205~$\pm$~38 &36.1   &$-$21.30  \\
\clvier &B5     &no  	&+5 &35  & $-$5	   &0.95     &300~$\pm$~79 &25.3   &$-$21.53  \\
\clvier &B6     &yes 	&+5 &40  &$-$15	   &0.25     &165~$\pm$~27 &17.1   &$-$20.41  \\
\clvier &B11    &yes 	&+3 &55  & 15	   &0.52     &180~$\pm$~23 &11.4   &$-$21.52  \\
\clvier &B12    &yes 	&+5 &43  &$-$75	   &0.30     &230~$\pm$~130&7.2	 &$-$20.42  \\
\clvier &B14    &yes 	&+3 &63  &$-$22	   &0.40     &220~$\pm$~27 &4.5	 &$-$20.00  \\
\hline 
\end{tabular}
\end{table}