\begin{table}%t1
\par
\caption{\label{sample.tab}General properties of the sample.}
%\centerline
 {\begin{tabular}{l l l l l l l l l }     % 7 columns
\hline\hline
                      % To combine 4 columns into a single one
Object          & $v$(km~s$^{-1}$)    & type & Bar-class$^{1}$& Nuclear type & Inner morph.$^{2}$&$B$& $V_{\rm max,gas}$  (km~s$^{-1}$\ )$^{3}$& $i$(deg)\\
\hline
NGC~1169$^{a}$   &  2387  & SABb    &3          & --             &   --         &12.35        & 259.1 $\pm$ 7.3              & 57.1 \\
NGC~1358        &  4028      & SAB(R)0    &    --       &Sy2           &   --         &13.19        & 136.1 $\pm$ 10.6              & 62.8 \\
NGC~1433$^{b}$   &1075        &(R)SB(rs)ab&4&Sy2&Double-bar$^{a}$&10.81& 85.1 $\pm$ 2.4 & 68.1\\
NGC~1530$^{b} $  &2461&SBb&6&--&--&12.50&169.1~$\pm$~3.5&58.3\\
NGC~1832$^{d}$   &1939&SB(r)bc&2&--&--&12.50&129.9~$\pm$~2.0& 71.8\\
NGC~2217        &1619  &(R)SB(rs)0/a&--&LINER?&Double-bar$^{b}$&11.36& 183.4~$\pm$ 9.2 & 30.7\\
NGC~2273$^{c}$  &1840&SB(r)a&2&Sy2&--&12.62&192.2~$\pm$~5.5&57.3\\
NGC~2523        &3471&SBbc&--&--&--&12.64 &211.4 $\pm$~10.9 &61.3\\
NGC~2665        &1734&(R)SB(r)a&--&--&--&12.47& 130.9~$\pm$~7.1&32.8\\
NGC~2681$^{c}$  &692&(R)SAB(rs)0/a&1&Sy3&Triple--bar$^{c}$&11.15&87.5~$\pm$~6.7&15.9\\
NGC~2859$^{c}$  &1687&(R)SB(r)0~\^&1&Sy&Double--bar$^{d}$&11.86& 238.5~$\pm$~13.3& 33.0\\
NGC~2935 & 2271 & (R)SAB(s)b  & --& -- &-- &12.26 &188.3~$\pm$~2.0 &42.7\\
NGC~2950       &1337&(R)SB(r)0\^~0&--&--&Double-bar$^{e}$&11.93& --& 62.0\\
NGC~2962       &1966&(R)SAB(rs)0&--&--&Double-bar$^{c}$&12.91&202.9~$\pm$~9.9& 72.7\\
NGC~3081$^{c}$  &2391&(R)SAB(r)0/a&3&Sy2&Double-bar$^{d}$&12.89 &99.9~$\pm$~4.0&60.1\\
NGC~4245$^{c}$  &815&SB(r)0/a&2&&--&12.33&113.5~$\pm$~5.4&56.1\\
NGC~4314$^{a}$  &963&SB(rs)a&3&LINER&Double-bar$^{c}$&11.42&253.3~$\pm$~24.6&16.2\\
NGC~4394$^{d}$  &922&(R)SB(r)b&3&LINER&--&11.59& 212.5~$\pm$~16.0&20.0\\
NGC~4643$^{c}$  &1335&SB(rs)0/a&3&LINER&--&11.68&171.4~$\pm$~7.2&42.9\\
NGC~5101$^{d}$  &1868&(R)SB(r)0/a&2&--&--&11.59&195.7~$\pm$~9.0&23.2\\
\hline
\end{tabular}}
\par
\smallskip
 { 
$(1):$ $^{a}$ Bar class derived from the $K$-band light distribution,  
Block et~al. (\cite{Block01});  
$^{b}$ Bar class derived from the $K$-band light distribution, Block et~al. (\cite{Block04});
$^{c}$ Bar class derived from the $K$-band light distribution, Buta et~al. 
(\cite{Buta06});
$^{d}$ Bar class derived from the $H$-band light distribution,
Laurikainen et~al. (\cite{Laurikainen04}).
$(2):$
$^{a}$~Buta (\cite{Buta86});
$^{b}$ Jungwiert (\cite{Jungwiert97});
$^{c}$ Erwin (\cite{Erwin04});
$^{d}$ Wozniak (\cite{Wozniak95}).
$(3)$ Rotational velocity corrected for inclination.}
\end{table}