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Table A.15:

Dereddened line intensity ratios with respect to I(H$\beta $) = 100 for knots analyzed in III Zw 107 (regions A, B, and C) and Tol 9 (spectra obtained with 2.5 m INT and 2.56 m NOT).
Line $f(\lambda)$ III Zw 107 A III Zw 107 B III Zw 107 C Tol 9 INT Tol 9 NOT
3554.42 He I 0.283 ... ... ... 3.8 $\pm$ 1.4 ...
3728.00 [O II] 0.256 213 $\pm$ 12 306 $\pm$ 23 20.32: 142 $\pm$ 10 177 $\pm$ 27
3770.63 H I 0.249 1.00: 0.54: ... 0.56: ...
3797.90 H I 0.244 2.37: ... ... 0.83: ...
3835.39 H I 0.237 3.60 $\pm$ 0.95 1.69: 5.02: 1.94: ...
3868.75 [Ne III] 0.230 23.3 $\pm$ 2.1 21.1 $\pm$ 4.0 20.64: 10.9 $\pm$ 2.0 12.08:
3889.05 H I 0.226 12.6 $\pm$ 1.7 11.1 $\pm$ 4.2 8.84: 6.9 $\pm$ 2.1 ...
3967.46 [NeIII]H7 0.210 17.1 $\pm$ 1.7 22.4 $\pm$ 2.9 ... 21.6 $\pm$ 1.9 ...
4068.60 [S II] 0.189 2.26 $\pm$ 0.82 4.69: ... 3.3 $\pm$ 1.1 ...
4101.74 H I 0.182 26.2 $\pm$ 1.8 26.1 $\pm$ 4.2 27.5 $\pm$ 6.5 25.3 $\pm$ 2.5 26.3 $\pm$ 4.0
4340.47 H I 0.127 46.7 $\pm$ 2.8 46.9 $\pm$ 4.8 47.5 $\pm$ 7.9 45.8 $\pm$ 3.2 46.9 $\pm$ 5.8
4363.21 [O III] 0.121 3.14 $\pm$ 0.67 1.97: ... 0.55: ...
4471.48 He I 0.095 4.08 $\pm$ 0.75 3.40: ... 3.94 $\pm$ 0.65 3.96:
4658.10 [Fe III] 0.050 1.06: ... ... 1.09: ...
4686.00 He II 0.043 ... ... ... 0.33: ...
4814.55 [Fe II] 0.012 ... ... ... 0.85: ...
4861.33 H I 0.000 100.0 $\pm$ 5.3 100.0 $\pm$ 8.2 100 $\pm$ 15 100.0 $\pm$ 6.0 100 $\pm$ 10
4921.93 He I -0.015 0.42: ... ... ... ...
4958.91 [O III] -0.024 123.7 $\pm$ 6.5 99.5 $\pm$ 8.1 93 $\pm$ 14 78.3 $\pm$ 5.2 75.5 $\pm$ 9.1
5006.84 [O III] -0.036 375 $\pm$ 18 293 $\pm$ 19 257 $\pm$ 32 236 $\pm$ 13 225 $\pm$ 21
5197.90 [N I] -0.082 1.08: 2.07: ... ... ...
5200.26 [N I] -0.083 0.36: ... ... 2.63 $\pm$ 0.78 ...
5517.71 [Cl III] -0.154 0.22: ... ... 0.57: ...
5537.88 [Cl III] -0.158 0.20: ... ... 0.64: ...
5754.64 [N II] -0.198 ... ... ... 0.41: ...
5875.64 He I -0.215 12.5 $\pm$ 1.1 13.1 $\pm$ 2.3 12.94: 12.6 $\pm$ 1.4 16.3 $\pm$ 3.8
6300.30 [O I] -0.282 4.56 $\pm$ 0.61 6.1 $\pm$ 2.0 7.57: 7.78 $\pm$ 0.71 7.32 $\pm$ 0.96
6312.10 [S III] -0.283 1.02 $\pm$ 0.23 ... ... 0.66: 0.66:
6363.78 [O I] -0.291 1.55 $\pm$ 0.42 2.01: 3.58: 2.14 $\pm$ 0.59 2.30 $\pm$ 0.91
6548.03 [N II] -0.318 9.98 $\pm$ 0.75 12.1 $\pm$ 1.4 13.6 $\pm$ 4.5 23.8 $\pm$ 1.8 24.3 $\pm$ 2.3
6562.82 H I -0.320 282 $\pm$ 16 273 $\pm$ 18 280 $\pm$ 35 267 $\pm$ 18 284 $\pm$ 30
6583.41 [N II] -0.323 28.7 $\pm$ 1.8 37.0 $\pm$ 3.2 41.4 $\pm$ 8.3 72.2 $\pm$ 4.9 82.1 $\pm$ 7.3
6678.15 He I -0.336 3.17 $\pm$ 0.50 4.01: ... 3.16 $\pm$ 0.64 4.1 $\pm$ 1.3
6716.47 [S II] -0.342 19.6 $\pm$ 1.3 36.4 $\pm$ 4.3 52.2 $\pm$ 8.7 37.0 $\pm$ 2.6 42.1 $\pm$ 3.9
6730.85 [S II] -0.344 15.9 $\pm$ 1.1 27.5 $\pm$ 3.6 35.6 $\pm$ 6.9 29.8 $\pm$ 2.2 35.7 $\pm$ 3.4
7065.28 He I -0.387 2.27 $\pm$ 0.40 ... ... 1.93 $\pm$ 0.51 2.41 $\pm$ 0.94
7135.78 [Ar III] -0.396 11.4 $\pm$ 0.9 9.4 $\pm$ 1.7 ... 10.5 $\pm$ 1.0 10.8 $\pm$ 1.5
7318.39 [O II] -0.418 2.12 $\pm$ 0.58 ... ... 1.96: 1.57 $\pm$ 0.43
7329.66 [O II] -0.420 2.48 $\pm$ 0.66 ... ... 1.08: 1.30 $\pm$ 0.34
7751.10 [Ar III] -0.467 ... ... ... ... 2.68 $\pm$ 0.68
Aperture size (arcsec)   7.2$\times$1 5.6$\times$1 5.2$\times$1 6.4$\times$1 3.8$\times$1
Distance (arcsec)a   - 7.2 12.4 - -
F(H$\beta $)b   22.3 $\pm$ 0.8 8.6 $\pm$ 0.4 1.56 $\pm$ 0.14 23.4 $\pm$ 0.9 3.8$\times$0.3
C(H$\beta $)   0.68 $\pm$ 0.04 0.15 $\pm$ 0.02 0.22 $\pm$ 0.03 0.50 $\pm$ 0.05 0.40 $\pm$ 0.05
$W_{\rm abs}$ (Å)   2.0 $\pm$ 0.3 1.30 $\pm$ 0.10 0.50 $\pm$ 0.10 7.5 $\pm$ 0.8 6.2 $\pm$ 0.6
-W(H$\alpha $) (Å)   306 $\pm$ 18 76 $\pm$ 5 30 $\pm$ 4 178 $\pm$ 12 186 $\pm$ 15
-W(H$\beta $) (Å)   44 $\pm$ 3 15 $\pm$ 2 4.7 $\pm$ 0.7 33 $\pm$ 2 17 $\pm$ 3
-W(H$\gamma$) (Å)   16.4 $\pm$ 1.0 5.5 $\pm$ 0.6 1.8 $\pm$ 0.3 12.3 $\pm$ 0.8  
-W([O III]) 5007 (Å)   172 $\pm$ 8 41 $\pm$ 3 11.6 $\pm$ 1.5 77 $\pm$ 4 32 $\pm$ 4

a Relative distance of the knot with respect to the main region in the galaxy; b in units of 10-15 erg s-1 cm-2 and not corrected for extinction.


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