\begin{table}%ta.7 online
\caption{\label{iras08208lineas}Dereddened line intensity ratios with respect to $I$(\Hb)~=~100 for regions analyzed in IRAS 08208+2816. The slit positions that we used for each knot are: PA~345$^{\circ}$ for C, PA 355$^{\circ}$ for \#8 and \#10, and PA 10$^{\circ}$ for \#3 y \#5.}
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{\small 
\begin{tabular}{l  r@{\hspace{5pt}}  r@{\hspace{8pt}}  r@{\hspace{8pt}}r@{\hspace{8pt}}r@{\hspace{8pt}}r@{\hspace{8pt}}  }
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  \hline \hline
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Line   & $f(\lambda)$&  C      & \#3 &     \#5 &      \#8          &    \#10\\
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 3728.00  [O  II] &   0.256 & 146.8 $\pm$ 9.8   &   279 $\pm$ 20    &   251 $\pm$ 24     &	   164 $\pm$ 22 	  &   324 $\pm$ 64    \\
 3750.15   H	I &   0.253 &  1.74  $\pm$  0.51  &	\nodata    &	    \nodata   &     \nodata 	  &	   \nodata  \\
 3770.63   H	I &   0.249 &  1.55  $\pm$  0.49  &	  \nodata  &	    \nodata   &     \nodata 	  &	   \nodata  \\
 3797.90   H	I &   0.244 &  2.86  $\pm$  0.60  &	 3.17:     &	    \nodata   &     \nodata  	  &	   \nodata  \\
 3835.39   H	I &   0.237 &  5.53  $\pm$  0.79  &	  \nodata  &	    \nodata         \nodata  	  &	   \nodata  \\
 3868.75 [Ne III] &   0.230 &  32.8  $\pm$  2.2   &  15.1  $\pm$  3.4   &  26.3  $\pm$  7.0    &       5.27:  	  &	   \nodata  \\
 3889.05   H	I &   0.226 &  15.1  $\pm$  1.7   &  13.5  $\pm$  3.2   &  12.9  $\pm$  5.0    &       6.36:  	  &	   \nodata  \\
 3967.46 [NeIII]H7&   0.210 &  22.1  $\pm$  1.9   &  15.9  $\pm$  2.9   &  17.0  $\pm$  5.3    &    22.0  $\pm$  5.7   &	26.23:      \\
 4026.21  He	I &   0.198 &	    0.92:     &	\nodata    &	    \nodata   &        \nodata    &	   \nodata  \\
 4068.60  [S  II] &   0.189 &  1.14  $\pm$  0.45  &	   \nodata &	    \nodata   &        \nodata    &	   \nodata  \\
 4101.74   H	I &   0.182 &  26.1  $\pm$  2.1   &  26.1  $\pm$  2.9   &  24.1  $\pm$  5.1    &  26.1  $\pm$  5.7  	  &	 26.23:     \\
 4340.47   H	I &   0.127 &  46.7  $\pm$  2.7   &  46.8  $\pm$  4.6   &  43.8  $\pm$  6.8    &  43.5  $\pm$  7.4  	  &    46  $\pm$  15    \\
 4363.21  [O III] &   0.121 &  3.12  $\pm$  0.48  &  1.66:          &	   2.26:      &	   \nodata  	  &	   \nodata  \\
 4471.48  He	I &   0.095 &  4.00  $\pm$  0.67  &   3.7  $\pm$  1.3   &	    \nodata   &        \nodata    &	   \nodata  \\
 4658.10 [Fe III] &   0.050 &  1.68  $\pm$  0.58  &       1.72:     &	    \nodata   &        \nodata    &	   \nodata  \\
% 4686.00  He   II &   0.043 &	    0.69:     &	 \nodata   &	    \nodata   &        \nodata    &	  \nodata    \\
 4861.33   H	I &   0.000 & 100.0  $\pm$  5.7   & 100.0  $\pm$  8.4   &   100  $\pm$  11     &	100  $\pm$  12   	  &   100  $\pm$  22    \\
 4958.91  [O III] &  --0.024 & 152.6  $\pm$  8.3   &  76.6  $\pm$  5.8   &   104  $\pm$  10     &  44.7  $\pm$  8.9  	  &    54  $\pm$  15    \\
 5006.84  [O III] &  --0.036 &	470  $\pm$  24    &   228  $\pm$  14    &   305  $\pm$  24     &	 89  $\pm$  13   	  &   151  $\pm$  30    \\
 5197.90  [N   I] &  --0.082 &  1.09  $\pm$  0.42  &	   \nodata &	   2.46:      &	    \nodata  	  &	   \nodata  \\
 5875.64  He	I &  --0.215 &  12.8  $\pm$  1.2   &  12.4  $\pm$  1.9   &  14.6  $\pm$  2.9    &  12.3  $\pm$  3.4  	  &	 11.28:     \\
 6300.30  [O   I] &  --0.282 &  4.74  $\pm$  0.62  &   5.6  $\pm$  1.1   &   9.8  $\pm$  2.3    &  10.1  $\pm$  3.1  	  &	  9.00:     \\
 6312.10  [S III] &  --0.283 &  1.46  $\pm$  0.42  &       1.13:     &	    \nodata   &        \nodata    &	   \nodata  \\
 6363.78  [O   I] &  --0.291 &  1.70  $\pm$  0.46  &	\nodata    &	   3.21:      &	   2.24:  	  &	   \nodata  \\
 6548.03  [N  II] &  --0.318 &  14.2  $\pm$  1.1   &  16.0  $\pm$  2.4   &  16.2  $\pm$  3.9    &  30.2  $\pm$  5.3  	  &	 14.95:     \\
 6562.82   H	I &  --0.320 &	285  $\pm$  15    &   283  $\pm$  20    &   281  $\pm$  25     &	288  $\pm$  33  	  &   286  $\pm$  51    \\
 6583.41  [N  II] &  --0.323 &  36.9  $\pm$  2.6   &  39.2  $\pm$  4.2   &  37.8  $\pm$  5.3    &  75.3  $\pm$  9.3  	  &    42  $\pm$  11    \\
 6678.15  He	I &  --0.336 &  3.26  $\pm$  0.63  &  3.04  $\pm$  0.93  &	    \nodata   &       2.93:  	  &	  3.65:     \\
 6716.47  [S  II] &  --0.342 &  22.0  $\pm$  1.5   &  40.2  $\pm$  4.2   &  52.9  $\pm$  6.8    &  66.4  $\pm$  9.6  	  &    50  $\pm$  13    \\
 6730.85  [S  II] &  --0.344 &  16.6  $\pm$  1.3   &  28.5  $\pm$  3.3   &  34.5  $\pm$  5.2    &  46.7  $\pm$  7.5  	  &    36  $\pm$  10    \\
 7065.28  He	I &  --0.387 &  2.42  $\pm$  0.57  &	   \nodata &	    \nodata   &      \nodata      &	   \nodata  \\
 7135.78 [Ar III] &  --0.396 &  6.37  $\pm$  0.78  &  11.8  $\pm$  3.0   &	    \nodata   &      \nodata  	  &	   \nodata  \\
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Aperture size (arcsec) & &   $1.4 \times 1$   &   $2.8 \times 1$   & $4.0 \times 1$    &  $6.4 \times 1$     &   $4.0 \times 1$ \\
Distance (arcsec)$^b$&      &       --          &   12.6           &  6.8             &     8.8           &    16   \\
$F$(\Hb)$^a$          &       & 12.9    $\pm$   0.5  & 5.97   $\pm$   0.28 &  2.98   $\pm$   0.19 &  4.05   $\pm$   0.34  & 1.36   $\pm$   0.18 \\ 
$C$(\Hb)              &       &  0.11   $\pm$   0.02 & 0.47   $\pm$   0.04 &  0.41   $\pm$   0.04 &  0.17   $\pm$   0.03  & 0.12   $\pm$   0.02 \\
$W_{\rm abs}$ (\AA)     &       &	3.2   $\pm$   0.1  & 1.6    $\pm$   0.2  &  1.4    $\pm$   0.2  &   4.9   $\pm$   0.1   & 1.9    $\pm$   0.1  \\ 
\noalign{\smallskip}					$-W$(\Ha) (\AA)     &       &   331   $\pm$   18   &  202   $\pm$   15   &   346   $\pm$     32 &    89   $\pm$   10    &   98   $\pm$    18  \\    
$-W$(\Hb) (\AA)     &       &    80   $\pm$    5   &   56   $\pm$    5   &	62   $\pm$      7 &    24   $\pm$    3    &   17   $\pm$     4  \\    
$-W$(H$\gamma$) (\AA)&      &    30   $\pm$    2  &   20   $\pm$    2   &	27   $\pm$      4 &    10   $\pm$    2    &    9   $\pm$     3  \\   
$-W$([O III]) (\AA)&   &   370  $\pm$  19  &    130  $\pm$   8   &   200  $\pm$    16 &    $18 \pm  3$    &   19  $\pm$    4  \\   
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$^a$ In units of 10$^{-15}$ erg s$^{-1}$ cm$^{-2}$ and not corrected for extinction; $^b$~relative distance with respect to the center of IRAS 08208+2816.
\end{table}