\begin{table}%t4 \caption{\label{table4}Rotational velocities of the sample.} %\centering \par \begin{tabular}{ccccccccccc} \hline \hline \noalign{\smallskip} & & & &\multicolumn{4}{c}{Observed} &\multicolumn{1}{c}{Model} \\ (1)&(2)&(3)&(4)&(5)&(6)&(7)&(8)&(9)&(10)&(11)\\ HCG& Galaxy & Morph.& $M{\rm_{B}}$ & $R_{25}$ & $V_{\rm{R(25)}}^{\rm{RC}}$ & $R_{\rm{max}}$ & $V_{\rm{max}}^{\rm{RC}}$ & $V_{\rm{R(25)}}^{\rm{model}}$ & $V_{\rm{max}}^{\rm{TF}}$ &$V_{\rm{max}}$ \\ &&Type&mag&(arcsec/kpc)&km s$^{-1}$& (arcsec/kpc) & km s$^{-1}$ & km s$^{-1}$ & km s$^{-1}$ & \\ \hline 2 &a & SBd & --20.75 &41/11.4&212&74/21.0& 264& 197 & 264 $\pm$ 39 & 1 \\ &b & cI & --19.39 &21/6.0 &...&7/2.0& 122& 270 & 196 $\pm$ 74 & 4 \\ &c & SBC & --19.87 &33/9.1 &118&40/11.2& 122& 106 & 122 $\pm$ 13 & 1 \\ 7 &a & Sb & --20.69 &57/15.3 &...&47/12.7& 226& 197 & 226 $\pm$ 27 & 2 \\ &d & SBC & --18.66 &38/10.1&...&16/4.3& 78 & 85 & 85 $\pm$ 4 & 2 \\ 22 &c & SBcd & --19.48 &52/8.3&143&52/8.3& 142& 142 & 142 $\pm$ 9 & 1 \\ 37 &d & SBdm & --18.65 &12/4.8&...&5/2.0& 63 & 76 & 76 $\pm$ 7 & 4 \\ 40 &c & Sbc & --19.91 &37/15.1&...&24/9.9& 197& 203 & 203 $\pm$ 3 & 2 \\ &e & Sc & --18.02 &18/7.3&...&7/2.9& 146& 226& 186 $\pm$ 40 & 4 \\ 47 &a & SBb & --21.23 &...&...&...& ...& ... & ...& ... \\ &d & Sd & --19.33 &...&...&...& ...& ... & ...& ... \\ 49 &a & Scd & --19.76 &14/9.4&...&10/6.4&126 & 182 & 154 $\pm$ 28 & 4 \\ &b & Sd & --19.47 &13/8.7&...&4/2.5&69 & 58 & 58 $\pm$ 6 & 3 \\ &c & Im & --18.36 &10/6.6&...&7/4.3&123 & 133 & 133 $\pm$ 5 &4 \\ 56 &a & Sc &--20.52 &28/15.2&200&22/12.0&205 & 228 & 205 $\pm$ 14 & 1 \\ 68 &c & SBbc & --20.83&77/12.6&244&115/18.9&244 & 234 & 244 $\pm$ 8 & 1 \\ 93 &b & SBd & --21.44 &57/17.7&191&28/8.5&235 & 220 & 235 $\pm$ 22 & 2 \\ &NGC 92 & Sa & --19.55&49/10.0 & ...&7/1.5&207 & 229 & 229 $\pm$ 11 & 4 \\ \hline \end{tabular} \tablefoot {Column (1): group number. Column~(2): Galaxy member of the group. Column~(3): morphological type taken from Hickson (\cite{Hick93b}). Column~(4): $B$-band absolute magnitude. Column~(5): isophotal radius at the limiting surface brightness of 25~B~mag~arcsec$^{-2}$, Column~(6): observed rotational velocity at~$R_{25}$. Column~(7): maximum radius reached by the rotation curve. Column~(8): observed maximum rotational velocity. Column~(9): rotational velocity at~$R_{25}$ derived from the arctan model. Column~(10): rotational velocity used in the TF~relation. Column~(11): quality flag on~$V_{\rm{max}}$ (1:~reached; 2:~probably reached; 3:~probably did not reach; 4:~did not~reach).} \vspace*{-3mm} \end{table}