\begin{table}%T5
\caption{General \hi~properties.}
\label{tab:hiprops}
\par
%\centerline
{
\begin{tabular}{lcccccccc}
\hline\hline
  & NGC~1406 & NGC~1511 & NGC~4244 & NGC~4565 & NGC~4666$^a$ 
  & NGC~4700 & NGC~7090 & NGC~7462 \\
\hline
$\alpha$(2000)$^b$  &  03:39:22.8 & 03:59:36.9 & 12:17:29.9 & 12:36:21.0 
  & 12:45:08.3 & 12:49:07.6 & 21:36:28.6 & 23:02:46.5 \\
%NED pos & ok & \~ok & ok & ok & \~ok & \~ok & ok & ok \\
$\delta$(2000)$^b$  & --31:19:16 & --67:38:08 & +37:48:31 & +25:59:13 
  & --00:27:51 & --11:24:47 & --54:33:24 & --40:50:05 \\
%NED pos & ok & \~ok & ok & ok & \~ok & \~ok & ok & ok \\
$D$ (Mpc)$^c$  & 14.9 & 17.5 & 3.0 & 9.7$^d$ & 26.4 & 25.5 & 11.7 & 15.1 \\
$v_{\rm hel}$ (km s$^{-1}$) & 1051 & 1335 & 244 & 1221 & 1520 & 1404 & 849 
  & 1064 \\
%NED Vhel & 1075! & 1329! & 244 & 1282X & 1520 & 1408 & 857! & 1059 \\
{PA} ($^\circ$) & 199 & 295 & 228 & 315 & 225 & 48 & 130 & 253 \\
{\it i} ($^\circ$) & 90$^e$ & 72$^e$ & 84.5$^f$ & $\geq$87.5$^g$ & 70 & 
  90$^e$ & 90$^e$ & 90$^e$ \\
$v_{\rm max}$ (km s$^{-1}$) & 171 & 150 & 113 & 271 & 180 & 87 & 124 & 112 \\
%RC3 v20 & 179 & 137! & 112 & 262 & 202 & 78 & 116 & 100 \\
$v_{\rm max}^{\rm i}$ (km s$^{-1}$) & 171 & 158 & 114 & 271 & 192 & 87 
  & 124 & 112 \\
$R_0$ (kpc) & 4.1 & 4.9 & 4.7 & 4.8 & 17 & 5.6 & 5.7 & 4.5 \\
%RC3 PA & 195! & 305! & 228! & 316! & 222! &  45! & 127! & 255 \\
$f_{\rm HI}$  (Jy~km~s$^{-1}$) & 62.3 & 44.3 & 379 & 249 & 93.5 & 21.7 
  & 39.8 & 32.7 \\
%NED f(HI) & 26-40 & 64-85 & 420-640 & 320 & 60-105 & 24-27 & 59 & 30-35 \\
$M_{\rm atom}$  ($10^{9}$ \msol) & 4.40 & 4.32 & 1.09 & 7.45 & 15.3 & 4.48 
  & 1.73 & 2.37 \\
\hline
\end{tabular}}
\par
\medskip
Notes (for details see text): \\
$^{a}$ Values from Walter et~al. (\cite{Walter04}). \\
$^{b}$ The kinematic centre positions were determined from rotation
curve fitting using routine {\sc rotcur}\ in {GIPSY}\ (see 
text). \\
$^{c}$ Distances are based on $H_0$ = 75 Mpc~km~s$^{-1}$ and a
virgocentric infall velocity of 300~km~s$^{-1}$ (cf. Dahlem et
al. \cite{Dahlem01}). \\
$^{d}$ The distance of NGC~4565 is hard to determine because of the
peculiar velocities of the Coma clouds (Ferrarese et~al. \cite{Ferrarese00}).
The value used here is from Tully (\cite{Tully88}). \\
$^{e}$ Tully (\cite{Tully88}). \\
$^{f}$ Olling (\cite{Olling96a}). \\
$^{g}$ Rupen (\cite{Rupen91}).
\end{table}