\begin{table}
%\centering
\par
 \caption{\label{wrgfotha}{Results of the \Ha\ photometry of the galaxies and regions analyzed in this work. The \Ha\ flux is corrected for both extinction and the contribution of the [\ion{N}{ii}] emission lines. Last column shows the age of the last starbursting episode derived  comparing \WHa\ with the predictions given by \citet{L99} models.}}
\begin{tabular}{l ccc ccc c}
\hline\hline
\noalign{\smallskip}
{\bf Object}     &   Flux    &      Luminosity     &    $M_{\rm H~ II}$     &	$M_{\star}$	&	 {\it SFR}	    &	  $W$(\Ha)     &  Age  \\
	   \noalign{\smallskip}
	          & (10$^{-13}$ erg cm$^{-2}$ s$^{-1}$) & (10$^{40}$ erg s$^{-1}$) & (10$^6$ \Mo) &  (10$^6$ \Mo)  & (\Mo\ yr$^{-1}$) & (\AA)& (Myr) \\
\hline
{\bf HCG 31} \\
      A1 &  0.137 $\pm$ 0.015 &  0.452 $\pm$ 0.049  &   0.067 $\pm$ 0.007 &   0.64 $\pm$ 0.07 & 0.036 $\pm$ 0.004 &  70 $\pm$  30 & 6.8 $\pm$ 0.6 \\
       B &  0.925 $\pm$ 0.078 &  3.05  $\pm$ 0.26   &   0.453 $\pm$ 0.038 &   8.20 $\pm$ 0.69 & 0.242 $\pm$ 0.020 &  80 $\pm$  20 & 6.5 $\pm$ 0.3 \\
AC$^b$   & 11.00  $\pm$ 0.70  & 36.3   $\pm$ 2.3    &   5.39  $\pm$ 0.34  &  18.2  $\pm$ 1.2  & 2.88  $\pm$ 0.18  & 500 $\pm$  40 & 4.9 $\pm$ 0.1 \\
       E &  0.452 $\pm$ 0.048 &  1.49  $\pm$ 0.16   &   0.222 $\pm$ 0.024 &   2.62 $\pm$ 0.28 & 0.118 $\pm$ 0.013 & 180 $\pm$  30 & 5.8 $\pm$ 0.2 \\
      F1 &  1.120 $\pm$ 0.070 &  3.70  $\pm$ 0.23   &   0.549 $\pm$ 0.034 &   0.87 $\pm$ 0.05 & 0.293 $\pm$ 0.018 &1200 $\pm$ 100 & 3.3 $\pm$ 0.2 \\
      F2 &  0.406 $\pm$ 0.024 &  1.34  $\pm$ 0.08   &   0.199 $\pm$ 0.011 &   0.28 $\pm$ 0.02 & 0.106 $\pm$ 0.006 &1100 $\pm$ 100 & 3.4 $\pm$ 0.2\\
       G &  1.95  $\pm$ 0.11  &  6.43  $\pm$ 0.36   &   0.955 $\pm$ 0.054 &   6.99 $\pm$ 0.39 & 0.511 $\pm$ 0.029 & 220 $\pm$  40 & 5.5 $\pm$ 0.3\\
       H &  0.014 $\pm$ 0.004 &  0.045 $\pm$ 0.013  &   0.007 $\pm$ 0.002 &   0.02 $\pm$ 0.01 & 0.004 $\pm$ 0.001 & 420 $\pm$ 100 & 4.8 $\pm$ 0.2\\
\hline
\noalign{\smallskip}
{\bf Mkn 1087}&  4.78  $\pm$ 0.33  & 70.0   $\pm$ 4.8   &  10.39   $\pm$ 0.72  & 129    $\pm$ 9    &   5.56  $\pm$ 0.38  &  90 $\pm$  20 & 6.2 $\pm$ 0.1 \\
           MB &  4.48  $\pm$ 0.31  & 65.6   $\pm$ 4.5   &   9.74   $\pm$ 0.67  &  85    $\pm$ 6    &   5.21  $\pm$ 0.36  & 150 $\pm$  20 & 6.0 $\pm$ 0.1 \\
          \#1 &  0.025 $\pm$ 0.007 &  0.365 $\pm$ 0.097 &   0.0541 $\pm$ 0.014 &   0.67 $\pm$ 0.18 &   0.029 $\pm$ 0.008 & 100 $\pm$  30 & 6.2 $\pm$ 0.2 \\
          \#7 &  0.274 $\pm$ 0.015 &  4.01  $\pm$ 0.22  &   0.596  $\pm$ 0.033 &   2.79 $\pm$ 0.15 &   0.319 $\pm$ 0.017 & 390 $\pm$  30 & 5.2 $\pm$ 0.2 \\
            N &  0.155 $\pm$ 0.013 &  2.27  $\pm$ 0.19  &   0.337  $\pm$ 0.028 &   3.34 $\pm$ 0.28 &   0.180 $\pm$ 0.015 &  80 $\pm$  20 & 6.5 $\pm$ 0.3\\
            K &  1.58  $\pm$ 0.09  & 23.1   $\pm$ 1.3   &   3.44   $\pm$ 0.20  &  30.1  $\pm$ 1.7  &   1.84  $\pm$ 0.11  & 180 $\pm$  30 & 5.8 $\pm$ 0.2\\
\par
\hline
\noalign{\smallskip}
\par
{\bf Haro 15}   &  4.66 $\pm$ 0.52 &  41.8 $\pm$ 4.7 &   6.21 $\pm$ 0.69 &  77 $\pm$ 9    &   3.32 $\pm$ 0.37 &  90 $\pm$  20 & 6.3 $\pm$ 0.3\\
 C         &  3.23 $\pm$ 0.42 &  29.0 $\pm$ 3.8 &   4.31 $\pm$ 0.56 &  53 $\pm$ 7    &   2.30 $\pm$ 0.30 & 110 $\pm$  20 & 6.2 $\pm$ 0.2\\
 A            &  1.27 $\pm$ 0.16 &  11.4 $\pm$ 1.4 &   1.69 $\pm$ 0.21 &  6.7 $\pm$ 0.8 &   0.91 $\pm$ 0.11 & 360 $\pm$  50 & 4.9 $\pm$ 0.2\\
 B             &  0.05 $\pm$ 0.02 &  0.50 $\pm$ 0.20 &  0.07 $\pm$ 0.03 &	1.8 $\pm$ 0.7 &   0.04 $\pm$ 0.01 &  60 $\pm$  25 & 7.0 $\pm$ 0.8\\
\par
\hline
\noalign{\smallskip}
{\bf Mkn 1199} &14.0 $\pm$ 2.1&   48.9 $\pm$ 7.3   &    7.3 $\pm$ 1.1  &    140 $\pm$ 21  &   3.9 $\pm$ 0.6   &  \nodata&  \nodata\\
     MB &   13.6 $\pm$ 2.0   &    47.5 $\pm$ 7.0   &    7.1 $\pm$ 1.0  &     84 $\pm$ 12  &   3.8 $\pm$ 0.6   &  \nodata&  \nodata\\
     NE &  0.259 $\pm$ 0.065 &    0.90 $\pm$ 0.23  &   0.13 $\pm$ 0.03 &   1.67 $\pm$ 0.42&   0.07 $\pm$ 0.02 &  \nodata&  \nodata\\
      A &  0.033 $\pm$ 0.010 &    0.12 $\pm$ 0.03  &   0.02 $\pm$ 0.01 &   0.70 $\pm$ 0.21&   0.01 $\pm$ 0.00 &  \nodata&  \nodata\\
      B &  0.064 $\pm$ 0.019 &    0.22 $\pm$ 0.07  &   0.03 $\pm$ 0.01 &   1.35 $\pm$ 0.40&   0.02 $\pm$ 0.01 &  \nodata&  \nodata\\
      e &  0.057 $\pm$ 0.017 &    0.20 $\pm$ 0.06  &   0.03 $\pm$ 0.01 &   1.20 $\pm$ 0.36&   0.02 $\pm$ 0.01 &  \nodata&  \nodata\\
\hline
\noalign{\smallskip}
{\bf Mkn 5}   &   3.00 $\pm$ 0.08  & 0.582 $\pm$ 0.014 &   0.081 $\pm$ 0.010  &  0.300 $\pm$ 0.012 &  0.046 $\pm$ 0.011 & 400 $\pm$  40 & 4.9 $\pm$ 0.2\\
          A   &   2.96 $\pm$ 0.08  & 0.510 $\pm$ 0.013 &   0.080 $\pm$ 0.010  &  0.290 $\pm$ 0.011 &  0.040 $\pm$ 0.010 & 442 $\pm$  66 & 4.8 $\pm$ 0.2\\
          B   &  0.042 $\pm$ 0.008 & 0.072 $\pm$ 0.014 &  0.0011 $\pm$ 0.0002 &  0.017 $\pm$ 0.002 &  0.006 $\pm$ 0.001 &  50 $\pm$  20 & 7.2 $\pm$ 0.8\\
\hline
\noalign{\smallskip}
{\bf IRAS 08208+2816}&3.29  $\pm$ 0.27  &  142 $\pm$ 12 &  21.1  $\pm$ 1.7  &    166 $\pm$ 14   &   11.3  $\pm$ 0.9   & 170 $\pm$  40 & 5.8 $\pm$ 0.3 \\
          \#1 &  0.046 $\pm$ 0.004 &  1.97  $\pm$ 0.18  &   0.29 $\pm$ 0.03 &   1.65 $\pm$ 0.15 &   0.156 $\pm$ 0.014 & 270 $\pm$  50 & 5.2 $\pm$ 0.2 \\
          \#2 &  0.058 $\pm$ 0.004 &  2.52  $\pm$ 0.18  &   0.34 $\pm$ 0.03 &   2.68 $\pm$ 0.19 &   0.200 $\pm$ 0.014 & 190 $\pm$  40 & 5.6 $\pm$ 0.3 \\
          \#3 &  0.219 $\pm$ 0.011 &  9.46  $\pm$ 0.48  &   1.41 $\pm$ 0.07 &   8.5  $\pm$ 0.4  &   0.75  $\pm$ 0.04  & 230 $\pm$  40 & 5.3 $\pm$ 0.3 \\
          \#4 &  0.031 $\pm$ 0.004 &  1.32  $\pm$ 0.16  &   0.20 $\pm$ 0.02 &   1.9  $\pm$ 0.2  &   0.105 $\pm$ 0.013 & 130 $\pm$  40 & 6.1 $\pm$ 0.3 \\
          \#5 &  0.279 $\pm$ 0.021 &  12.1  $\pm$ 0.9   &   1.79 $\pm$ 0.13 &   8.0  $\pm$ 0.6  &   0.96  $\pm$ 0.07  & 330 $\pm$  40 & 5.0 $\pm$ 0.2 \\
       \#6(C) &  1.29  $\pm$ 0.07  &  56    $\pm$ 3     &    8.3 $\pm$ 0.5  &   35.0 $\pm$ 1.9  &   4.43  $\pm$ 0.24  & 350 $\pm$  50 & 5.0 $\pm$ 0.1 \\
          \#7 &  0.032 $\pm$ 0.005 &  1.38  $\pm$ 0.21  &   0.21 $\pm$ 0.03 &   1.5  $\pm$ 0.2  &   0.110 $\pm$ 0.016 & 180 $\pm$  50 & 5.7 $\pm$ 0.4 \\
          \#8 &  0.170 $\pm$ 0.017 &  7.35  $\pm$ 0.74  &   1.09 $\pm$ 0.11 &  12.5  $\pm$ 1.3  &   0.58  $\pm$ 0.06  & 110 $\pm$  30 & 6.2 $\pm$ 0.3 \\
          \#9 &  0.067 $\pm$ 0.010 &  2.91  $\pm$ 0.44  &   0.43 $\pm$ 0.06 &    5.9 $\pm$ 0.9  &   0.23  $\pm$ 0.04  &  90 $\pm$  20 & 6.4 $\pm$ 0.4 \\
         \#10 &  0.106 $\pm$ 0.012 &  4.58  $\pm$ 0.52  &   0.68 $\pm$ 0.08 &    7.8 $\pm$ 0.9  &   0.36  $\pm$ 0.04  & 110 $\pm$  30 & 6.2 $\pm$ 0.3 \\
\hline
\noalign{\smallskip}
\par
{\bf IRAS 08339+6517}$^b$ & 16.0 $\pm$ 0.7  & 120 $\pm$ 6   & 14.5 $\pm$ 0.7  &  226 $\pm$ 10  & 9.5 $\pm$ 0.5 & 110 $\pm$ 10 & 6.0 $\pm$ 0.2\\
Companion             & 0.28 $\pm$ 0.03 & 2.1 $\pm$ 0.4 & 0.26 $\pm$ 0.03 &  4.1 $\pm$ 0.5 & 0.17 $\pm$ 0.02 & 31 $\pm$ 5 & 6.7 $\pm$ 0.2\\
\hline
\noalign{\smallskip}
\par
{\bf POX 4} &  15.5  $\pm$ 0.5   &   38.4 $\pm$ 1.2  &   5.70 $\pm$ 0.18 &	9.77 $\pm$ 0.32 &   3.05 $\pm$ 0.10 & 910 $\pm$ 5   & 4.5 $\pm$ 0.1 \\
     \#3 &  0.675 $\pm$ 0.027 &  1.67 $\pm$ 0.07 &   0.25 $\pm$ 0.01 &	0.54 $\pm$ 0.02 &   0.13 $\pm$ 0.01 & 840 $\pm$  10 & 4.6 $\pm$ 0.2 \\
     \#6 &  0.380 $\pm$ 0.030 &  0.94 $\pm$ 0.07 &   0.14 $\pm$ 0.01 &	0.24 $\pm$ 0.02 &   0.07 $\pm$ 0.01 &1110 $\pm$  25 & 4.0 $\pm$ 0.2 \\
     \#7 &  0.033 $\pm$ 0.004 &  0.08 $\pm$ 0.01 &   0.01:           &	0.05 $\pm$ 0.01 &   0.01:           & 415 $\pm$  20 & 5.0 $\pm$ 0.2 \\
  \#9-C  &  11.2  $\pm$ 0.4   &   27.8 $\pm$ 1.0  &   4.12 $\pm$ 0.15 &	7.06 $\pm$ 0.25 &   2.20 $\pm$ 0.08 &1410 $\pm$   5 & 3.1 $\pm$ 0.1 \\
    \#11 &  0.178 $\pm$ 0.011 &  0.44 $\pm$ 0.03 &   0.07:           &	0.25 $\pm$ 0.02 &   0.04:           & 450 $\pm$  10 & 5.0 $\pm$ 0.1 \\
     Comp&  0.127 $\pm$ 0.011 &  0.31 $\pm$ 0.03 &   0.05:           &	0.79 $\pm$ 0.07 &   0.02:           & 320 $\pm$   5 & 5.2 $\pm$ 0.2 \\
\hline
\noalign{\smallskip}
\par
{\bf UM 420} &  0.695 $\pm$ 0.043  &   46.8 $\pm$ 2.9  &   6.95 $\pm$ 0.43 &   13.75 $\pm$ 0.85 &   3.71 $\pm$ 0.23 & 980 $\pm$  60 & 4.3 $\pm$ 0.2 \\
\hline
\noalign{\smallskip}
\par
{\bf SBS 0926+606  A}  & 2.52 $\pm$ 0.12  &  9.43 $\pm$ 0.45 &   1.40 $\pm$ 0.07 &	3.59 $\pm$ 0.17 &   0.75 $\pm$ 0.04 & 600 $\pm$  40 & 4.8 $\pm$ 0.2 \\
  A1                   & 1.46 $\pm$ 0.11  &  5.46 $\pm$ 0.41 &   0.81 $\pm$ 0.06 &	2.08 $\pm$ 0.16 &   0.43 $\pm$ 0.03 & 670 $\pm$  50 & 4.7 $\pm$ 0.2 \\
  A2                   & 1.06 $\pm$ 0.09  &  3.96 $\pm$ 0.34 &   0.59 $\pm$ 0.05 &	1.51 $\pm$ 0.13 &   0.31 $\pm$ 0.03 & 510 $\pm$  60 & 4.9 $\pm$ 0.2 \\
{\bf SBS 0926+606  B}  & 0.631 $\pm$ 0.056 & 2.36 $\pm$ 0.21 &   0.35 $\pm$ 0.03 &	4.76 $\pm$ 0.42 &   0.19 $\pm$ 0.02 & 130 $\pm$  20 & 6.7 $\pm$ 0.3 \\
  Bc                   & 0.327 $\pm$ 0.031 & 1.22 $\pm$ 0.12 &   0.18 $\pm$ 0.02 &	2.47 $\pm$ 0.23 &   0.10 $\pm$ 0.01 & 220 $\pm$  40 & 5.9 $\pm$ 0.3 \\
\hline
{\bf SBS 0948+532} &   1.86 $\pm$ 0.07  &  78.2 $\pm$ 2.9    &  11.61 $\pm$ 0.44 &  18.84 $\pm$ 0.71 &   6.21 $\pm$ 0.23  & 810 $\pm$  30& 4.6 $\pm$ 0.2 \\
\hline
 {\bf SBS 1054+365} &   5.87 $\pm$ 0.22  &  0.450 $\pm$ 0.017 &   0.067$\pm$0.003 &	0.23 $\pm$ 0.01 &  0.036 $\pm$ 0.001 & 320 $\pm$  50 & 5.2 $\pm$ 0.2 \\
    C &   5.16 $\pm$ 0.15  &  0.395 $\pm$ 0.011 &   0.059$\pm$0.002 &	0.20 $\pm$ 0.01 &  0.031 $\pm$ 0.001 & 490 $\pm$  40 & 4.9 $\pm$ 0.1 \\
    a &   1.30 $\pm$ 0.060 &  0.100 $\pm$ 0.005 &   0.015$\pm$0.001 &	0.05:           &  0.008:            & 390 $\pm$  40 & 5.0 $\pm$ 0.2 \\
    b1 &  0.062 $\pm$ 0.009 &  0.005 $\pm$ 0.001 &   \nodata         &	0.02:           &  \nodata           &  40 $\pm$  15 & 9.8 $\pm$ 1.0 \\
    b2 &  0.062 $\pm$ 0.009 &  0.005 $\pm$ 0.001 &   \nodata         &	0.02:           &  \nodata           &  25 $\pm$  20 & 11  $\pm$ 2 \\
     e &  0.734 $\pm$ 0.041 &  0.056 $\pm$ 0.003 &   0.008:          &	0.03:           &  0.004:            & 270 $\pm$  40 & 5.5 $\pm$ 0.3 \\
     \hline
{\bf SBS 1211+540} &  0.817 $\pm$ 0.031 &  0.141 $\pm$ 0.005 &   0.021~$\pm$~0.001 &	0.05:           &  0.011:            & 640 $\pm$  40 & 4.8 $\pm$ 0.2\\
     C &  0.726 $\pm$ 0.026 &  0.125 $\pm$ 0.004 &   0.019~$\pm$~0.001 &	0.04:           &  0.010:            & 730 $\pm$  50 & 4.7 $\pm$ 0.2\\
     a &  0.610 $\pm$ 0.030 &  0.105 $\pm$ 0.005 &   0.016~$\pm$~0.001 &	0.04:           &  0.008:            & 490 $\pm$  60 & 5.0 $\pm$ 0.2\\
\hline
\noalign{\smallskip}
 {\bf SBS 1319+579}  & 2.40 $\pm$ 0.15  &   2.38 $\pm$ 0.15 &    0.354 $\pm$ 0.022  &  0.78 $\pm$ 0.05 &0.189 $\pm$ 0.012 & 620 $\pm$  60& 4.9 $\pm$ 0.2\\
        A &  1.480 $\pm$ 0.008 &  1.469 $\pm$ 0.008 &   0.2182 $\pm$ 0.0012 &   0.28 $\pm$ 0.02 &	0.117 $\pm$ 0.001 &1300 $\pm$  80& 3.6 $\pm$ 0.4 \\
        B &  0.107 $\pm$ 0.009 &  0.106 $\pm$ 0.009 &   0.0158 $\pm$ 0.0013 &   0.10 $\pm$ 0.01 &	0.008 $\pm$ 0.001 & 150 $\pm$  30& 6.5 $\pm$ 0.4\\
        C &  0.579 $\pm$ 0.041 &  0.575 $\pm$ 0.041 &   0.0854 $\pm$ 0.0060 &   0.28 $\pm$ 0.02 &	0.046 $\pm$ 0.003 & 320 $\pm$  40& 5.3 $\pm$ 0.3 \\
 {\it d} &  0.056 $\pm$ 0.005 &  0.056 $\pm$ 0.005 &   0.0083 $\pm$ 0.0008 &   0.06 $\pm$ 0.01 &	0.004             & 120 $\pm$  30& 7.1 $\pm$ 0.5\\
 {\it e} &  0.024 $\pm$ 0.003 &  0.024 $\pm$ 0.003 &   0.0035 $\pm$ 0.0004 &   0.03            &	0.002             & 100 $\pm$  30& 7.3 $\pm$ 0.8\\
 {\it f} &  0.081 $\pm$ 0.006 &  0.080 $\pm$ 0.006 &   0.0119 $\pm$ 0.0008 &   0.07            &	0.006             & 220 $\pm$  30& 5.9 $\pm$ 0.4\\
 {\it g} &  0.026 $\pm$ 0.003 &  0.026 $\pm$ 0.003 &   0.0038 $\pm$ 0.0004 &   0.04            &	0.002             &  90 $\pm$  30& 7.3 $\pm$ 0.9\\
 {\it i} &  0.010 $\pm$ 0.002 &  0.010 $\pm$ 0.001 &   0.0015 $\pm$ 0.0002 &   0.02            &	0.001             &  50 $\pm$  20& 9.1 $\pm$ 1.1\\	 
\hline
\noalign{\smallskip}	 
{\bf  SBS 1415+437} & 4.78 $\pm$ 0.20& 0.495 $\pm$ 0.021&   0.0735 $\pm$ 0.0031 &  0.14 $\pm$ 0.01 & 0.039 $\pm$ 0.002 & 900 $\pm$  60 & 4.5 $\pm$ 0.2\\
     Main Body &  4.66 $\pm$ 0.19  &  0.482 $\pm$ 0.020 &   0.0716 $\pm$ 0.0029 &  0.11            & 0.038 $\pm$ 0.002 & 900 $\pm$  60 & 4.5 $\pm$ 0.2\\
            C &  4.10 $\pm$ 0.16   &  0.424 $\pm$ 0.017 &   0.0630 $\pm$ 0.0025 &  0.10            & 0.034 $\pm$ 0.001 &1250 $\pm$  60 & 3.7 $\pm$ 0.3\\
            A &  0.465 $\pm$ 0.022 &  0.048 $\pm$ 0.002 &   0.0071 $\pm$ 0.0003 &  0.02            & 0.004             &1100 $\pm$  60 & 4.0 $\pm$ 0.3\\
            B &  0.121 $\pm$ 0.009 &  0.013 $\pm$ 0.001 &   0.0019 $\pm$ 0.0001 &  0.01            & 0.001             & 200 $\pm$  30 & 6.1 $\pm$ 0.2\\
     {\it d} &  0.096 $\pm$ 0.008 &  0.010 $\pm$ 0.001 &   0.0015 $\pm$ 0.0001 &  \nodata         & 0.001             & 550 $\pm$  50 & 4.9 $\pm$ 0.2\\
\hline
\noalign{\smallskip}
{\bf III Zw 107} &  5.29 $\pm$ 0.24   & 40.1 $\pm$ 1.8   &   5.96   $\pm$ 0.27  &  73.9 $\pm$ 3.4  &  3.19 $\pm$ 0.15   & 160 $\pm$  30 & 5.9 $\pm$ 0.3 \\
             A &  4.22 $\pm$ 0.18   & 32.0 $\pm$ 1.4   &   4.75   $\pm$ 0.20  &  32.5 $\pm$ 1.4  &  2.54 $\pm$ 0.11   & 250 $\pm$  40 & 5.6 $\pm$ 0.3 \\
             B &  0.965 $\pm$ 0.046 &  7.32 $\pm$ 0.35 &   1.087  $\pm$ 0.052 &  44.4 $\pm$ 2.1  &  0.58 $\pm$ 0.03   &  80 $\pm$  30 & 6.5 $\pm$ 0.5 \\
             C &  0.101 $\pm$ 0.018 &  0.77 $\pm$ 0.14 &   0.114  $\pm$ 0.020 &   5.6 $\pm$ 1.00 &  0.061 $\pm$ 0.011 &  40 $\pm$  20 & 7.6 $\pm$ 1.4 \\
\hline
\noalign{\smallskip}		 
{\bf Tol 9} & 10.2   $\pm$ 0.7   & 22.9   $\pm$ 1.6    &   3.4    $\pm$ 0.2    &  27.4  $\pm$ 1.9  &   1.82  $\pm$ 0.13  & 130 $\pm$  30 & 6.0 $\pm$ 0.3 \\
     C &  8.5   $\pm$ 0.4   & 19.0   $\pm$ 1.0    &   2.83   $\pm$ 0.14   &  40    $\pm$ 2    &   1.51  $\pm$ 0.08  & 200 $\pm$  30 & 5.8 $\pm$ 0.2 \\
   \#1 &  0.027 $\pm$ 0.002 &  0.061 $\pm$ 0.005  &   0.0091 $\pm$ 0.0007 &   0.13 $\pm$ 0.01 &   0.005 $\pm$ 0.001 & 110 $\pm$  30 & 6.1 $\pm$ 0.2 \\
   \#2 &  0.105 $\pm$ 0.006 &  0.236 $\pm$ 0.013  &   0.035  $\pm$ 0.002  &   0.50 $\pm$ 0.03 &   0.019 $\pm$ 0.001 & 180 $\pm$  30 & 5.8 $\pm$ 0.2 \\
   \#3 &  0.031 $\pm$ 0.004 &  0.070 $\pm$ 0.009  &   0.0104 $\pm$ 0.0013 &   0.15 $\pm$ 0.02 &   0.006 $\pm$ 0.001 & 110 $\pm$  40 & 6.2 $\pm$ 0.2 \\
   \#4 &  0.020 $\pm$ 0.003 &  0.045 $\pm$ 0.008  &   0.0066 $\pm$ 0.0011 &   0.09 $\pm$ 0.02 &   0.004 $\pm$ 0.001 & 140 $\pm$  40 & 6.0 $\pm$ 0.2 \\
   \#5 &  0.31  $\pm$ 0.04  &  0.69  $\pm$ 0.09   &   0.102  $\pm$ 0.013  &   1.46 $\pm$ 0.19 &   0.055 $\pm$ 0.007 & 120 $\pm$  40 & 6.1 $\pm$ 0.3 \\
   \#6 &  0.002:            &  0.003:             &   0.0005:             &   0.01:           &   \nodata           &  80 $\pm$  30 & 6.3 $\pm$ 0.3 \\
{\it Env}& 0.45  $\pm$ 0.04  &  1.017 $\pm$ 0.09   &   0.151  $\pm$ 0.013  &   \nodata       &   \nodata &   \nodata   & \nodata \\
\hline
\noalign{\smallskip}	
{\bf Tol 1457-262}& 11.4 $\pm$ 0.6& 63.3 $\pm$ 3.5   &   9.4    $\pm$ 0.5    &  41    $\pm$ 2    &	5.0   $\pm$ 0.3   & 340 $\pm$  50 & 5.1 $\pm$ 0.2 \\
\noalign{\smallskip}
Obj 1 &  8.33  $\pm$ 0.49  & 46.2   $\pm$ 2.7   &   6.9    $\pm$ 0.4    &  23.4  $\pm$ 1.4  &	3.7   $\pm$ 0.2   & 430 $\pm$  40 & 4.9 $\pm$ 0.2 \\
  \#1 &  0.354 $\pm$ 0.032 &  1.97  $\pm$ 0.18  &   0.29   $\pm$ 0.03   &   2.09 $\pm$ 0.19 &	0.156 $\pm$ 0.014 & 190 $\pm$  30 & 5.8 $\pm$ 0.3 \\
  \#2 &  0.319 $\pm$ 0.028 &  1.77  $\pm$ 0.16  &   0.26   $\pm$ 0.02   &   1.59 $\pm$ 0.14 &	0.141 $\pm$ 0.012 & 230 $\pm$  40 & 5.4 $\pm$ 0.3 \\
\#3(B)&  0.854 $\pm$ 0.049 &  4.74  $\pm$ 0.27  &   0.70   $\pm$ 0.04   &   2.60 $\pm$ 0.15 &	0.38  $\pm$ 0.02  & 410 $\pm$  40 & 5.0 $\pm$ 0.2 \\
  \#4 &  0.444 $\pm$ 0.040 &  2.47  $\pm$ 0.22  &   0.37   $\pm$ 0.03   &   1.82 $\pm$ 0.16 &	0.196 $\pm$ 0.018 & 290 $\pm$  40 & 5.2 $\pm$ 0.3 \\
  \#5 &  0.550 $\pm$ 0.043 &  3.05  $\pm$ 0.24  &   0.45   $\pm$ 0.04   &   1.57 $\pm$ 0.12 &	0.242 $\pm$ 0.019 & 440 $\pm$  50 & 4.9 $\pm$ 0.2 \\
\#6(A)&  3.20  $\pm$ 0.22  & 17.8   $\pm$ 1.2   &   2.64   $\pm$ 0.18   &   8.1  $\pm$ 0.6  &	1.4   $\pm$ 0.1   & 650 $\pm$  50 & 4.6 $\pm$ 0.2 \\
\#7(C)&  0.621 $\pm$ 0.050 &  3.45  $\pm$ 0.28  &   0.51   $\pm$ 0.04   &   1.71 $\pm$ 0.14 &	0.27  $\pm$ 0.02  & 320 $\pm$  40 & 5.1 $\pm$ 0.2 \\
  \#8 &  0.482 $\pm$ 0.039 &  2.68  $\pm$ 0.22  &   0.40   $\pm$ 0.03   &   2.41 $\pm$ 0.19 &	0.212 $\pm$ 0.017 & 230 $\pm$  40 & 5.4 $\pm$ 0.3 \\
\noalign{\smallskip}  
Obj 2 &  3.10  $\pm$ 0.14  & 17.21  $\pm$ 0.78  &   2.56   $\pm$ 0.12   &  14.4  $\pm$ 0.7  &	1.37  $\pm$ 0.06  & 250 $\pm$  30 & 5.2 $\pm$ 0.2 \\
  \#9 &  0.623 $\pm$ 0.036 &  3.46  $\pm$ 0.20  &   0.51   $\pm$ 0.03   &   3.8  $\pm$ 0.2  &	0.275 $\pm$ 0.016 & 180 $\pm$  30 & 5.7 $\pm$ 0.2 \\
 \#10 &  0.833 $\pm$ 0.042 &  4.62  $\pm$ 0.23  &   0.69   $\pm$ 0.03   &   4.2  $\pm$ 0.2  &	0.367 $\pm$ 0.019 & 230 $\pm$  40 & 5.4 $\pm$ 0.2 \\
 \#11 &  0.339 $\pm$ 0.024 &  1.88  $\pm$ 0.13  &   0.28   $\pm$ 0.02   &   2.60 $\pm$ 0.18 &	0.149 $\pm$ 0.011 & 140 $\pm$  30 & 6.0 $\pm$ 0.3 \\
 \#12 &  0.495 $\pm$ 0.038 &  2.75  $\pm$ 0.21  &   0.41   $\pm$ 0.03   &   2.16 $\pm$ 0.17 &	0.218 $\pm$ 0.017 & 270 $\pm$  40 & 5.2 $\pm$ 0.2 \\
 \#13 &  0.244 $\pm$ 0.022 &  1.35  $\pm$ 0.12  &   0.20   $\pm$ 0.02   &   1.76 $\pm$ 0.16 &	0.108 $\pm$ 0.010 & 150 $\pm$  30 & 6.0 $\pm$ 0.2 \\
 \#14 &  0.204 $\pm$ 0.014 &  1.13  $\pm$ 0.078 &   0.168  $\pm$ 0.012  &   1.32 $\pm$ 0.09 &	0.090 $\pm$ 0.006 & 170 $\pm$  30 & 5.8 $\pm$ 0.2 \\
\noalign{\smallskip}
 \#15 &  0.085 $\pm$ 0.007 &  0.474 $\pm$ 0.039 &   0.070  $\pm$ 0.006  &   0.80 $\pm$ 0.07 &	0.038 $\pm$ 0.003 &  90 $\pm$  20 & 6.4 $\pm$ 0.4 \\
 \#16 &  0.006 $\pm$ 0.002 &  0.036 $\pm$ 0.010 &   0.005  $\pm$ 0.002  &   0.10 $\pm$ 0.03 &	0.003 $\pm$ 0.001 &  60 $\pm$  30 & 7.0 $\pm$ 1.0 \\
\hline
\noalign{\smallskip}	
{\bf Arp 252}& 4.48 $\pm$ 0.30& 90.3 $\pm$ 6.1   &  13.4    $\pm$ 0.9    &  82.3  $\pm$ 4.9  &	7.2   $\pm$ 0.5   & \nodata	      & \nodata \\
ESO 566-8&  4.17  $\pm$ 0.28  & 84.1   $\pm$ 5.6   &  12.5    $\pm$ 0.8    &  45.1  $\pm$ 3.0  &	6.68  $\pm$ 0.45  & 440 $\pm$  40 & 4.9 $\pm$ 0.3 \\
      a1 &  3.82  $\pm$ 0.19  & 77.0   $\pm$ 3.8   &  11.4    $\pm$ 0.6    &  37.2  $\pm$ 1.9  &	6.12  $\pm$ 0.30  & 510 $\pm$  40 & 4.2 $\pm$ 0.4 \\
      a2 &  0.085 $\pm$ 0.007 &  1.72  $\pm$ 0.15  &   0.26  $\pm$ 0.02  &   0.85 $\pm$ 0.08 &	0.136 $\pm$ 0.012 & 460 $\pm$  50 & 4.8 $\pm$ 0.6 \\
      \hline
ESO 566-7&  0.312 $\pm$ 0.022 &  6.3  $\pm$ 0.4  &   0.93  $\pm$ 0.07    &  16.8  $\pm$ 1.2  &	0.50  $\pm$ 0.04  &  90 $\pm$  20 & 6.1 $\pm$ 0.2 \\
      b1 &  0.165 $\pm$ 0.010 &  3.3  $\pm$ 0.2  &   0.49   $\pm$ 0.03   &   8.9  $\pm$ 0.5 &	0.264 $\pm$ 0.016 & 130 $\pm$  20 & 5.9 $\pm$ 0.2 \\
      b2 &  0.140 $\pm$ 0.011 &  2.8  $\pm$ 0.2  &   0.419  $\pm$ 0.033  &   7.5  $\pm$ 0.6 &	0.224 $\pm$ 0.018 &  80 $\pm$  20 & 6.2 $\pm$ 0.2 \\
      b3 &  0.008 $\pm$ 0.002 &  0.17 $\pm$ 0.04 &   0.025  $\pm$ 0.007  &   0.44 $\pm$ 0.12 &	0.013 $\pm$ 0.004 &  50 $\pm$  20 & 6.4 $\pm$ 0.3 \\
       c &  0.017 $\pm$ 0.003 &  0.34 $\pm$ 0.06 &   0.051  $\pm$ 0.009  &   0.92 $\pm$ 0.16 &	0.027 $\pm$ 0.005 & 500 $\pm$ 100 & 4.5 $\pm$ 0.8 \\
       d &  0.008 $\pm$ 0.003 &  0.16 $\pm$ 0.05 &   0.024  $\pm$ 0.008  &   0.43 $\pm$ 0.13 &  0.013 $\pm$ 0.004 &  50 $\pm$  20 & 6.4 $\pm$ 0.3 \\
\hline
\noalign{\smallskip}	
{\bf NGC 5253}$^c$   &   229 $\pm$ 11 &  4.39 $\pm$ 0.21 &  0.651 $\pm$ 0.031 &   2.22 $\pm$ 0.11 &   0.348 $\pm$ 0.017 & 450 $\pm$  5 & 5.0 $\pm$ 0.1\\
\hline
  \end{tabular}
\par
\smallskip
\par
 $^a$ HCG 31AC is NGC 1741.\\ 
 $^b$ Values extracted from \citet{LSEGR06}.\\
 $^c$ Data of the \Ha\ flux and $W$(\Ha) extracted from \citet{Meurer06}.\\ 
  \end{table}