\begin{table}%t3
\caption{\label{table3}Kinematic properties of the sample}
%\centering
\par
\begin{tabular}{cccccccccccc}
\hline \hline \noalign{\smallskip}
 (1)&(2)&(3)&(4)&(5)&(6)&(7)&(8)&(9)&(10)&(11)&(12)\\ 
HCG & Galaxy & PA$_{\rm{kin}}$ & PA$_{\rm{morph}}$ & PA$_{\rm{morph}}$
&$i_{\rm{kin}}$ &$i_{\rm{morph}}$ & $i_{\rm{morph}}$ &$V_{\rm{sys HICK}}$ & $V_{\rm{sys FP}}$&
{\it vvir} & $\delta$ $c_{\rm{kin-morph}}$\\ & & deg & deg & deg & deg & deg &
deg &km s$^{-1}$ & km s$^{-1}$& km s$^{-1}$ & arcsec\\
\hline
2
&a &  42 $\pm$ 4 & 3 & 8 $\pm$ 13   & 68 $\pm$ 13 & 61 $\pm$ 2 & 65 & 4326 & 4347& 4375  &42.2\\
&b &  5 $\pm$ 3 & 28  & 3 $\pm$ 90   & 49 $\pm$ 12 &  30 $\pm$ 21  & 43 & 4366  & 4357&  4365 &1.3\\
&c &  168 $\pm$ 4 & 132 & 158 $\pm$ 18 & ... &   57 $\pm$ 3 & 64 & 4235 & 4266& 4284  &2.4 \\
7
&a &  179 $\pm$ 2 & 153 & 165 $\pm$ 13  & 67 $\pm$ 3 & 61 $\pm$ 2  &  76 & 4210& 4198& 4178   &0.6\\
&d &  85 $\pm$ 3 & 58  & 35 $\pm$ 34   & 31 $\pm$ 12  & 43 $\pm$ 7 &   44 & 4116&4104&  4081 &12.3\\
22
&c &  101 $\pm$ 2 & 70  & 179 $\pm$ 90 & ...  &  25 $\pm$ 14 & 90  & 2728 & 2572  & 2444 &6.8\\
37
&d   &  68 $\pm$ 4 & 58  & 108 $\pm$ 90 &  60 $\pm$ 15 & 38 $\pm$ 29 &36 & 6207 & 6308& 6236 &0.8\\
40
&c   &  120 $\pm$ 2 & 125 &  134 $\pm$ 8 & 74 $\pm$ 4  &  75 $\pm$ 2 &90  & 6890 & 6888& 6341 &1.6\\
&e   &  8 $\pm$ 10 & 72  &  57 $\pm$ 21 &  ... & 70 $\pm$ 6  & 80 & 6625 & ...&  6383  &0.0\\
47
&a   & 42 $\pm$ 3 & 42 & 14 $\pm$ 25  &  24 $\pm$ 11 & 47 $\pm$ 5 &  67 &9581 & 9507 & 9622   &...\\
&d   & 15 $\pm$ 1 & 165& 174 $\pm$ 54 & 16 $\pm$ 4  & 39 $\pm$ 12 &  32 & 9471 & 9325& 9533&...\\
49
&a   & 42 $\pm$ 8 & 57 & 49 $\pm$ 90 & 18 $\pm$ 10  & 22 $\pm$ 23 &  43 &9939 & 9812& 10196 &9.1\\
&b   & 91 $\pm$ 3  & 72 & 85 $\pm$ 31 &  51 $\pm$ 7 & 49 $\pm$ 7  & 59 & 9930& 9787& 10190&4.5\\
&c   & 175 $\pm$ 4 & 98 & 100 $\pm$ 90 &  11 $\pm$ 6 & 39 $\pm$ 31  & 45 & 9926& 9784& 10185 &23.7\\
56
&a   & 174 $\pm$ 1 & 172 & 173 $\pm$ 7  & 75 $\pm$ 3  & 75 $\pm$ 1  &  90  & 8245& 8374&8455  &1.6\\
68
&c   & 31 $\pm$ 1 & 119 & 34 $\pm$ 25   & 30 $\pm$ 4  & 36 $\pm$ 4 &  54 & 2313 & 2515& 2550 &1.0\\
93
&b   & 173 $\pm$ 4 & 156 & 39 $\pm$ 8  &  79 $\pm$ 6 & 70 $\pm$ 1 &  68 & 4672 & 4625& 4776 &1.3\\
&NGC 92 & 146 $\pm$ 2 & 149 & 149 $\pm$ 12 & 48 $\pm$ 6 & 63/62 $\pm$ 2 & 70 & 3219 & 3412 & 3132 &0.7\\
\hline
\end{tabular}
\tablefoot {Column (1): group number. Column~(2): Galaxy member of the group. Column~(3): PA deduced from our velocity field. Column~(4): PA taken from \mbox{Mendes de Oliveira} (\cite{Mend92}) for HCG. This was determinated for semimajor axis lengths of 2~$h^{-1}$~kpc for all Hickson group galaxies with $z$~$\leq$~0.05. Column~(5): optical~PA taken from HyperLeda. PA~is the position angle of the major axis of the isophote 25~mag~arcsec$^{-2}$ in the $B$-band. Column~(6): inclination deduced from the analysis of our velocity field. Column~(7): morphological inclination deduced from the axis ratio of the isophote 25~mag~arcsec$^{-2}$ in the $B$-band for galaxies ($\rm{cos}\it{(b/a)}=\it{i}$). For~NGC~92 given values correspond to HyperLeda/NED. Column~(8): morphological inclination taken from HyperLeda. Column~(9): systemic velocity taken from Hickson (\cite{Hick93b}). Column~(10): systemic velocity deduced from our velocity field analysis. Column~(11): radial velocity corrected by the Virgo infall from HyperLeda. Column~(12): difference in arcseconds between the morphologial and kinematic centers.}
\vspace*{1.5mm}
\end{table}