\begin{table}%t2
\caption{\label{tab:THINGS}Observed properties of the analyzed THINGS galaxies.}
%\centerline
{
\begin{tabular}{rrccccccccc}
\hline\hline\\[-0.3cm]
& Hubble & $D$ & $v_{\rm rot}$       & $R_{25}$ & $M_{\rm HI}$               & $\dot{M}_{\rm SF}$      & $\langle \sigma \rangle$ & $\langle \Sigma_{\rm HI} \rangle$ &   $\langle L_{\rm d} \rangle_{\rm HD}$ & $\langle L_{\rm d} \rangle_{\rm pot}$ \\
          & type  & Mpc&  km$~$s$^{-1}$ & kpc     & $10^9~$$M_{\odot}$ & $M_{\odot}$~yr$^{-1}$ & km$~$s$^{-1}$ & $M_{\odot}$~pc$^{-2}$    &kpc       & kpc \\
Name &{\em (1)} & {\em (2)} & {\em (3)} & {\em (4)} & {\em (5)} & {\em (6)} & {\em (7)} & {\em (8)} & {\em (9)} & {\em (10)}  ~\\
\hline  
% name         vrot     r25    MHI(e9)   SFR     <sigma>  <Sdens>   <Ld>      Ein       <Edecay>   epsilon   
NGC 5194 &   Sbc  &  8.0 &    220 &   9.0 &    2.5 &   6.05 &  31.69 &   7.18 &   4.72 &   1.32   \\ 
 NGC 628 &   ~Sc  &  7.3 &    220 &  10.4 &    3.8 &   1.21 &  14.28 &   4.55 &   1.00 &    0.80 \\ 
NGC 3184 &   ~Sc  & 11.1 &    210 &  11.9 &    3.1 &   1.43 &  18.34 &   4.48 &   1.46 &    0.99 \\ 
NGC 3351 &   ~Sb  & 10.1 &    200 &  10.6 &    1.2 &   0.71 &  20.89 &   2.05 &   5.42 &     1.01 \\ 
NGC 6946 &   ~Sc  &  5.9 &    200 &   ~9.8 &    4.2 &   4.76 &  18.72 &   5.57 &   1.28 &    1.13 \\ 
NGC 5055 &   Sbc  & 10.1 &    200 &  17.2 &    9.1 &   2.42 &  23.58 &   3.15 &   4.15 &    2.81\\ 
NGC 4736 &   Sab  &  4.7 &    160 &   ~5.3 &    0.4 &   0.43 &  24.98 &   2.99 &   5.11 &     0.71 \\ 
NGC 7793 &   Scd  &  3.9 &    130 &   ~6.0 &    0.9 &   0.51 &  19.64 &   6.06 &   1.40 &     0.91 \\ 
 IC 2574 &   ~Sm  &  4.0 &     80 &   ~7.5 &    1.5 &   0.12 &  17.30 &   5.82 &   1.13 &     2.42 \\ 
NGC 4214 &   Irr  &  2.9 &     60 &   ~2.9 &    0.4 &   0.05 &  16.91 &   4.78 &   1.18 &     1.17\\ 
   HO II &   Irr  &  3.4 &     40 &   ~3.3 &    0.6 &   0.07 &  16.89 &   6.37 &   0.96 &     1.99 \\ 
\hline
\end{tabular}}
\tablefoot{{\em (1)} Hubble type as listed in the LEDA data base (URL: \protect\url{http://leda.univ-lyon1.fr/}). {\em (2)} Distance according to \citet{Walter:2008p2669}. {\em (3)} Peak of the rotation curve as obtained from the  Appendix in \citet{deBlok:2008p4057}. {\em (4)} $R_{25}$ is the $B$-band isophotal radius at 25~mag~arcsec$^{-2}$, which is a standard proxy for the optical radius of the galaxy. {\em (5)} Total HI mass of the galaxy, obtained by integrating over all pixels, see also Table 4 of \citet{Leroy:2008p4217}.~ {\em (6)} Total star formation rate of the galaxy, as provided by Table 1 of \citet{Walter:2008p2669} or Table~4 of \citet{Leroy:2008p4217}. {\em (7)} Surface-density weighted 3-dimensional mean velocity dispersion in the galaxy. {\em (8)} Mean HI surface density. {\em (9)}~Typical outer scale of the turbulent velocity field. $\langle L_{\rm d} \rangle_{\rm HD}$ is calculated from the disk thickness in each pixel as  $L_{\rm d} = 2 H$ with $H = \sigma_{\rm 1D}^2 / (2 \pi G \Sigma_{\rm HI})$ and then averaged over the entire galaxy using surface-density weighting.~ {\em (10)} Estimate of the mean turbulent dissipation scale $\langle L_{\rm d} \rangle_{\rm pot}$ based on the disk thickness derived from the potential method, Eq.~(\ref{eqn:total-pot}). }
\end{table}