\begin{table}%ta.3 online %\centering \par \caption{\label{mkn1199lineas}Dereddened line intensity ratios with respect to $I$(\Hb)=100 for knots analyzed in Mkn 1199.} %\centerline {\small \begin{tabular}{l r rrrrr} \noalign{\smallskip} \hline \hline \noalign{\smallskip} Line & $f(\lambda)$& $C$ & NE & $A$ & $B$ & $D$ \\ \noalign{\smallskip} \tableline \noalign{\smallskip} 3728.00 [O II] & 0.256 & $124.6\pm7.8$ & $254\pm20$ & 204: & 145: & $192\pm45$\\ 3835.39 H I & 0.237 & 1.23: & \nodata & \nodata & \nodata & \nodata\\ 3868.75 [Ne III] & 0.230 & $1.39\pm0.46$ & 6.64: & \nodata & \nodata & \nodata\\ 3889.05 H I & 0.226 & $9.2\pm1.9$ & 9.40: & \nodata & \nodata & \nodata\\ 3967.46 [Ne III] & 0.210 & \nodata & 6.22: & \nodata & \nodata & \nodata\\ 3970.07 H I & 0.210 & $18.0\pm1.2$ & \nodata & \nodata & \nodata & \nodata\\ 4101.74 H I & 0.182 & $27.0\pm1.9$ & $26.0 \pm 5.9$& \nodata & \nodata & $30.5\pm7.6$\\ 4340.47 H I & 0.127 & $45.9\pm3.4$ & $46.7\pm6.2$ & 31: & \nodata & $47\pm18$ \\ % 4363.21 [O III] & 0.121 & 0.17: & \nodata & \nodata & \nodata & \nodata\\ 4471.48 He I & 0.095 & 2.48: & 5.46: & \nodata & \nodata & \nodata\\ 4658.10 [Fe III] & 0.050 & $3.44\pm0.68$ & \nodata & \nodata & \nodata & \nodata\\ 4686.00 He II & 0.043 & 0.24: & \nodata & \nodata & \nodata & \nodata\\ 4861.33 H I & 0.000 & $100.0\pm6.0$ & $100\pm11$ & 100: & 100: & $100\pm27$ \\ 4958.91 [O III] & --0.024 & $10.7\pm1.4$ & $60.0\pm8.4$ & 23: & \nodata & 23.5: \\ 5006.84 [O III] & --0.036 & $30.6\pm2.4$ & $167\pm15$ & 62: & 85: & $60\pm20$ \\ 5055.98 Si II & --0.048 & 0.81: & 2.37: & \nodata & \nodata & \nodata\\ 5197.90 [N I] & --0.082 & $2.49\pm0.60$ & \nodata & \nodata & \nodata & \nodata\\ 5754.64 [N II] & --0.194 & 0.61: & \nodata & \nodata & \nodata & \nodata\\ 5875.64 He I & --0.215 & $9.46\pm0.93$ & $12.7\pm3.1$ & \nodata & \nodata & 11.6:\\ 6300.30 [O I] & --0.282 & $3.57\pm0.80$ & $6.6\pm2.4$ & \nodata & \nodata & 16.8:\\ 6312.10 [S III] & --0.283 & 0.14: & 1.19: & \nodata & \nodata & \nodata\\ 6363.78 [O I] & --0.291 & 0.85: & \nodata & \nodata & \nodata & \nodata\\ 6548.03 [N II] & --0.318 & $48.2\pm3.1$ & $13.9\pm3.5$ & 51: & 51: & $57\pm14$ \\ 6562.82 H I & --0.320 & $293\pm17$ & $290\pm25$ & 294: & 296: & $298\pm65$ \\ 6583.41 [N II] & --0.323 & $149.8\pm8.9$ & $41.2\pm5.6$ & 142: & 141: & $172\pm35$ \\ 6678.15 He I & --0.336 & $1.90\pm0.49$ & 3.88: & \nodata & \nodata & \nodata\\ 6716.47 [S II] & --0.342 & $35.8\pm2.3$ & $35.4\pm5.2$ & 66: & 74: & $74\pm19$ \\ 6730.85 [S II] & --0.344 & $32.1\pm6.4$ & $25.5\pm4.4$ & 40: & 44: & $49\pm14$ \\ 7065.28 He I & --0.387 & $1.30\pm0.42$ & \nodata & \nodata & \nodata & \nodata\\ 7135.78 [Ar III] & --0.396 & $1.91\pm0.56$ & 6.29: & \nodata & \nodata & \nodata\\ 7318.39 [O II] & --0.418 & $0.87\pm0.32$ & \nodata & \nodata & \nodata & \nodata\\ 7329.66 [O II] & --0.420 & 0.39: & \nodata & \nodata & \nodata & \nodata\\ \noalign{\smallskip} \tableline \noalign{\smallskip} Aperture size (arcsec) & & 10 $\times$ 1 & 6 $\times$ 1 & 8 $\times$ 1 & 8 $\times$ 1 & 5.6 $\times$ 1\\ Distance$^b$ (arcsec) & & 0 & 26 & 18 & 14 & 8.4 \\ $F$(\Hb)$^a$ & & 74.2 $\pm$ 3.1 & 3.17 $\pm$ 0.21 & 0.33 $\pm$ 0.08 & 0.42 $\pm$ 0.10 & 0.98 $\pm$ 0.14 \\ $C$(\Hb) & & 0.30 $\pm$ 0.03 & 0.16 $\pm$ 0.03 & 0.17 $\pm$ 0.04 & 0.44 $\pm$ 0.06 & 0.27 $\pm$ 0.04 \\ $W_{\rm abs}$ (\AA) & & 1.8 $\pm$ 0.4 & 0.6 $\pm$ 0.3 & 1.7 $\pm$ 0.3 & 2 & 2.5 $\pm$ 0.3 \\ \noalign{\smallskip} $-W$(\Ha) (\AA) & & 129.1 $\pm$ 7.9 & 110 $\pm$ 10 & 21 $\pm$ 7 & 22 $\pm$ 8 & 34.7 $\pm$ 7.6 \\ $-W$(\Hb) (\AA) & & 21.4 $\pm$ 1.3 & 20.2 $\pm$ 2.3 & 5.0 $\pm$ 2.6 & 5.2 $\pm$ 2.4 & 8.3 $\pm$ 2.3 \\ $-W$(H$\gamma$) (\AA)& & 6.7 $\pm$ 0.5 & 8.4 $\pm$ 1.1 & 1.5 $\pm$ 1.7 & \nodata & 2.1 $\pm$ 0.8 \\ $-W$([O III]) 5007 (\AA)& & 6.8 $\pm$ 0.5 & 35.5 $\pm$ 3.4 & 2.8 $\pm$ 1.6 & 4.2 $\pm$ 1.8 & 5.1 $\pm$ 1.7 \\ \noalign{\smallskip} \tableline \end{tabular}} \medskip $^a$ In units of 10$^{-15}$~erg~s$^{-1}$ cm$^{-2}$ and not corrected for extinction; $^b$~relative distance with respect to the center of Mkn~1199. \end{table}