\begin{table}%T2
\caption{\label{table2}Derived parameters of the \hi~cores.}
\small%\centering
\par
\begin{tabular}{c c c c c c c c}
\hline\hline
          &$N_{\rm HI}$ & $s$  &$D$  & $T_{\rm kin}$&  $\langle n \rangle $ &   $P$    &  $M_{\hi}$  \\
          & \unith & arcmin  & pc &  K       & ${\rm cm^{-3}}$ &  $K~{\rm cm^{-3}}$ & \msun    \\
\hline 
Range     &12--32  &58--127    &1.9--5.9  &140--350 & 1.3--3.1& 270--980 & 1--24 \\
Median      &16  &  78      &2.6 & 240       &  2.3   & 560    & 4  \\ 
Range     &29--76& 54-124     &2--6 &170--730  & 2.2--5.7  &780--2440&7--32 \\
Median      & 40  &   86     & 5   &   410  & 3.6       & 1500   &16   \\
\hline
\end{tabular}
\tablefoot{The first two rows correspond to  the cloud 116.2+23.6 observed with WSRT. The last two rows  correspond to the cloud 115.0+23.9 observed with VLA. $N_{\rm HI}$  is the observed \hi\
  column density of the cores, $s$  is the angular size, $D$  is the spatial
  diameter. $T_{\rm kin}$   is the kinetic temperature. $\langle n \rangle $~ is
  the volume \hi~density. $P$ is the pressure of the \hi~gas. $M_{\hi}$ is
  the visible \hi~mass of the core. }
\end{table}