\begin{table}%T7 
  \caption{\label{masas}Keplerian mass (\Mkep), dynamical mass (\Mdyn), neutral gas mass (\MHi), ionized gas mass (\MHii), warm dust mass (\Mdust),  
mass of the ionizing star cluster (\Mstar), total stellar mass ($M_{\rm stars}$), and baryonic mass (\Mbar) of the galaxies analyzed in this work.}
\small%\centering
\par
  \begin{tabular}{l  cc  cc cc  cc}
  \hline\hline 
   \noalign{\smallskip}
Galaxy      &   \Mkep     &  \Mdyn &      \MHi   &        \MHii    &    \Mdust &   \Mstar     & $M_{\rm stars}$  & \Mbar  \\
            & [10$^8$~\Mo]& [10$^8$~\Mo]& [10$^8$~\Mo]& [10$^6$~\Mo]& [10$^6$~\Mo] & [10$^6$~\Mo] & [10$^8$~\Mo] & [10$^8$~\Mo] \\		    
\hline  
   HCG 31    & \nodata   &  \nodata&  74.6         &  7.8~$\pm$~0.5  &  2.56      &  37.8~$\pm$~2.8  &   33.8   & 141  \\
   $''$      AC &  340      &  850    &  36.4 	       &  5.4~$\pm$~0.3  &   \nodata  &  18.2~$\pm$~1.2	 &   14.4   &  62.5   \\
   $''$      B  &   26      &   54	   &  19.4	       &  0.45~$\pm$~0.04&   \nodata  &   8.2~$\pm$~0.7  &    8.0   &  33.6    \\
   $''$      E  & \nodata   & 13\tablefootmark{a}  & \nodata       &  0.22~$\pm$~0.02&   \nodata  &   2.6~$\pm$~0.3 &    0.47   & \nodata\\
   $''$      F  &    3.0    &   15	   &   6.13	       &  0.75~$\pm$~0.04&   \nodata  &  0.40~$\pm$~0.03 &   0.39  &   8.5 \\
   $''$      G  &   21      &   68	   &  19.4	       &  0.96~$\pm$~0.05&   \nodata  & 	7.0~$\pm$~0.4  &   10.5  &   36.1   \\
   Mkn 1087  &  560      & 1800    & 156           &  10.4~$\pm$~9.7 &    7.8     &   129~$\pm$~9    &   288   &  494  \\
   $''$       N &   2.2     & 45\tablefootmark{a}  & \nodata       & 0.337~$\pm$~0.028& \nodata   &  3.34~$\pm$~0.28 &     4.0 & \nodata\\
   Haro 15   &  121      &  365    &  55~$\pm$~18    &  6.2~$\pm$~0.7  &    2.1     & 	77~$\pm$~9     &   99.2  &  172   \\
   Mkn 1199  &   82      & 1650    &  12.2	       &  7.3~$\pm$~1.1  &    3.1     &   140~$\pm$~21   &   275   &  291   \\
   $''$ NE      &  2.9      &  70\tablefootmark{a} & \nodata       &  0.13~$\pm$~0.03& \nodata    &   1.7~$\pm$~0.4  &   17.4  & \nodata\\
   Mkn 5     &   21      &   36	   & 0.72~$\pm$~0.09 & 0.081~$\pm$~0.010&   0.099   &0.300~$\pm$~0.012 &    1.5  &   2.5 \\
IRAS 08208+2816&  39     & 600\tablefootmark{a} & \nodata       &  21.1~$\pm$~1.7 &    8.84    &  166~$\pm$~14    &   298   & \nodata\\
IRAS 08339+6517&  100    &  370	   &  53~$\pm$~6     &  14.5~$\pm$~0.7 &    3.91    &  226~$\pm$~10    &   476   &  546   \\
$''$ Comp       &     80    &  100    &  7.0~$\pm$~0.9  &  0.26~$\pm$~0.03& \nodata    &  4.1~$\pm$~0.5   &   18.6  &  27.9    \\ 
POX 4        &    5.0    &   76	   &  21	       &  5.70~$\pm$~0.18&    0.093   &  9.8~$\pm$~0.3   &   14.3  &  29.1   \\
$''$ Comp       & \nodata   & \nodata & \nodata       &   0.05         & \nodata   &  0.79~$\pm$~0.07 &   0.88  & \nodata \\
	UM 420   &   21      &  200\tablefootmark{a} & \nodata       &  6.9~$\pm$~0.4  &    5.0\tablefootmark{b} & 13.8~$\pm$~0.9   &   45.6  & \nodata\\
SBS 0926+606 &  \nodata  & \nodata & 17.7~$\pm$~7.2  &  1.75~$\pm$~0.10&    0.37    & 8.4~$\pm$~0.6    &  7.59   &  30.9 \\  
$''$ A          &  \nodata  &     23  &  9.6~$\pm$~3.6  &  1.40~$\pm$~0.07&   \nodata  & 3.59~$\pm$~0.17  &    2.9  &  15.5   \\
$''$ B          &  \nodata  &     45  &  8.1~$\pm$~3.6  &  0.35~$\pm$~0.03&   \nodata  &  4.8~$\pm$~0.4   &    4.7   & 15.4   \\
SBS 0948+532 &   21      &  90\tablefootmark{a}  & \nodata       &  11.6~$\pm$~0.4 &   \nodata  & 18.8~$\pm$~0.7   &   12.6 &\nodata\\
SBS 1054+365 &    0.78   &    15   &  0.61~$\pm$~0.06&0.067~$\pm$~0.003&    0.012   & 0.23~$\pm$~0.01  &    0.33 &    1.13 \\
SBS 1211+540 &    1.13   &     1.14&  0.24~$\pm$~0.04&0.021~$\pm$~0.001&   \nodata  & 	 0.05	     &  0.102 & 0.420  \\
SBS 1319+579 &   86      &  140    & 16.4          &  0.35~$\pm$~0.02&    0.30    & 0.78~$\pm$~0.05  &   22.9   &  44.5   \\
SBS 1415+437 &    2.5    &    4.9  &  0.96~$\pm$~0.07& 0.074~$\pm$~0.003&  \nodata  & 0.14~$\pm$~0.01  &    0.46 &    1.74 \\
  III Zw 107 &    8.2    &  180	   &  67~$\pm$~12    &  6.0~$\pm$~0.3  &    1.25    & 	74~$\pm$~3     &   61.8  &  150   \\
      Tol 9  &   12      & 580 &  22~$\pm$~2     &  3.4~$\pm$~0.2  &    2.41    &  27.4~$\pm$~1.9  &   44.4   &  106   \\
Tol 1457-262 &   \nodata & 950     &  47	       &  9.4~$\pm$~0.5  &    1.83    &  41~$\pm$~2      &   87.2   &  149   \\
$''$ Obj 1      & 62        & 290\tablefootmark{a} &  \nodata	   &  6.9~$\pm$~0.4  &    \nodata &  23.4~$\pm$~1.5  &   46.9   &  \nodata   \\
$''$ Obj 2      &  \nodata  & 150\tablefootmark{a} &  \nodata      & 2.56~$\pm$~0.12 &  \nodata   &  14.4~$\pm$~0.7  &   36.2  &  \nodata \\
Arp 252      & \nodata   &\nodata  &  \nodata      &  13.4~$\pm$~0.9 &   6.32     & 82.3~$\pm$~4.9   & 338    & \nodata \\
$''$ ESO 566-8    &   73      & 440\tablefootmark{a} & \nodata     & 12.5~$\pm$~0.8  & \nodata    &  45~$\pm$~3      &  250   & \nodata\\
$''$ ESO 566-7    &    4      & 150\tablefootmark{a} & \nodata     & 0.93~$\pm$~0.07 & \nodata    &  16.8~$\pm$~1.2  &   88   & \nodata\\
NGC 5253     & \nodata   &  83 & 1.59~$\pm$~0.09 & 0.65~$\pm$~0.03 &  0.042     &  2.22~$\pm$~0.11 &   11.4   &   13.5   \\
\hline
  \end{tabular}
 \tablefoot{\tablefoottext{a}{Tentative value of \Mdyn\ computed using Eqs.~(\ref{emdynmb})$-$(\ref{emdynmj}) and~(\ref{ecmdyn}).}\\
  \tablefoottext{b}{The warm dust mass is very probably overestimated because of the \FIR\ contribution by the foreground galaxy~UGC~01809.}} 
\end{table}