\begin{table}%t1
%\centering
\par
\caption{Parameters of the sample galaxies.} \label{t1}
\begin{tabular}{lllrrccrrc}
\hline \hline
\noalign{\smallskip} 
\multicolumn{1}{c}{Name} & 
\multicolumn{2}{c}{Morphological type} &
\multicolumn{1}{c}{PA} & 
\multicolumn{1}{c}{$V_\odot$} & 
\multicolumn{1}{c}{$D$} & 
\multicolumn{1}{c}{$M^0_{B_{\rm T}}$} & 
\multicolumn{1}{c}{$D_{25} \times d_{25}$} &
\multicolumn{1}{c}{$i$} &  
\multicolumn{1}{c}{Minor-axis region} \\
\noalign{\smallskip}
\multicolumn{1}{c}{} &  
\multicolumn{1}{c}{[RSA]} & 
\multicolumn{1}{c}{[RC3]} & 
\multicolumn{1}{c}{[$^\circ$]} &
\multicolumn{1}{c}{[km s$^{-1}$]} & 
\multicolumn{1}{c}{[Mpc]} &
\multicolumn{1}{c}{[mag]} & 
\multicolumn{1}{c}{} & 
\multicolumn{1}{c}{[$^\circ$]} &
\multicolumn{1}{c}{where $V_{\rm g}\neq0$} \\
\noalign{\smallskip}
\multicolumn{1}{c}{(1)} &
\multicolumn{1}{c}{(2)} & 
\multicolumn{1}{c}{(3)} & 
\multicolumn{1}{c}{(4)} & 
\multicolumn{1}{c}{(5)} & 
\multicolumn{1}{c}{(6)} & 
\multicolumn{1}{c}{(7)} & 
\multicolumn{1}{c}{(8)} &
\multicolumn{1}{c}{(9)} & 
\multicolumn{1}{c}{(10)}\\ 
\noalign{\smallskip} 
\hline 
\noalign{\smallskip} 
NGC~1638& Sa                & SAB0(rs)?    &  70& $3258\pm11$& 43.5& $-20.42$& $2\farcm0\times1\farcm5$& 43& ?\\ 
NGC~2855& Sa(r)             & (R)S0/a(rs)  & 120& $1897\pm17$& 22.3& $-19.45$& $2\farcm5\times2\farcm2$& 27& inner\\
NGC~3885& Sa                & S0/a(s)      & 123& $1952\pm 8$& 22.3& $-19.44$& $2\farcm4\times1\farcm0$& 69& inner\\
NGC~4224& Sa                & Sa(s): sp    &  57& $2624\pm 6$& 33.0& $-20.07$& $2\farcm6\times1\farcm0$& 69& inner\\
NGC~4235& Sa                & Sa(s) sp     &  48& $2249\pm11$& 28.1& $-20.35$& $4\farcm2\times0\farcm9$& 82& ?\\
NGC~4586& Sa                & Sa(s): sp    & 115&  $815\pm 7$& 17.0& $-19.04$& $4\farcm0\times1\farcm3$& 73& inner\\
NGC~4984& Sa(s)             & (R)SAB0$^{+}$&  90& $1279\pm 6$& 14.2& $-18.73$& $2\farcm8\times2\farcm2$& 38& extended\\
NGC~7049& S0$_{3}$(4)/Sa    & S0(s)        &  57& $2285\pm 6$& 29.6& $-20.79$& $4\farcm3\times3\farcm0$& 47& inner\\
NGC~7213& Sa(rs)            & Sa(s):       & 124& $1784\pm 6$& 23.1& $-20.69$& $3\farcm1\times2\farcm8$& 27& extended\\
NGC~7377& S0$_{2/3}$/Sa pec & S0$^{+}$(s)  & 101& $3339\pm11$& 45.7& $-21.37$& $3\farcm0\times2\farcm5$& 34& extended\\ 
\hline 
\end{tabular}  
%
Notes. -- 
Column 2: morphological classification from RSA.
Column 3: morphological classification from RC3.
Column 4: major-axis position angle from RC3. 
Column 5: heliocentric systemic velocity derived from the center of 
        symmetry of the rotation curve of the gas along the
        galaxy major axis.
Column 6: distance obtained as $V_0/H_0$ with $H_0=75$~\kmsmpc\ 
        and $V_0$ the systemic velocity derived from $V_\odot$ 
        corrected for the motion of the Sun with respect of the 
        Local Group according to the RSA. For NGC 4586 we assumed 
        the distance of the Virgo Cluster by Freedman et~al. (\cite{Fre94}).
Column 7: absolute total blue magnitude corrected for 
        inclination and extinction from RC3.
Column 8: major and minor isophotal diameters from RC3.
Column 9: inclination derived from $\cos^{2}{i}~=~(q^2-q_0^2)/(1-q_0^2)$ 
        assuming the observed axial ratio $q=d_{25}/D_{25}$ from RC3
        and the typical intrinsic axial ratio for S0/Sa and Sa galaxies 
        ($q_0=0.18$, Guthrie \cite{Gut92}).  
Column 10: minor-axis region where non-zero velocity is measured for
         the ionized gas. Inner = non-zero velocity is 
         confined to the nuclear region; extended = non-zero velocity is
         observed out to the last measured radius; ? = doubtful velocity 
         gradient.
\end{table}