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Table 4:

Calculated total column densities of the observed interstellar features.
HD/Obs N(OH) N(CH) N(CH+) N(CN) N(H2)
  [1012 cm-2] [1012 cm-2] [1012 cm-2] [1012 cm-2] [1020 cm-2]
23180 B 39.00 a 22.24 $\pm $ 2.91 7.89 $\pm $ 0.63 1.82 $\pm $ 0.12 4.00g
24398 B 40.50 $\pm $ 4.00b 22.30 $\pm $ 2.61 4.28 $\pm $ 1.84 3.12 $\pm $ 0.18 4.70g
27778 B 102.00 $\pm $ 4.00b 39.93 $\pm $ 4.10 10.55 $\pm $ 0.63 26.76 $\pm $ 4.12f 6.17h
34078 G/B 35.00$\pm $ 4.00c 79.27 $\pm $ 4.82 57.28 $\pm $ 2.25 $^{d^{\prime}}$ 2.16 $\pm $ 0.05 6.40c
147889 u 252.36 $\pm $ 30.74 100.33 $\pm $ 5.87 33.90 $\pm $ 1.96d 25.06 $\pm $ 2.09e  
148688 u 23.11 $\pm $ 9.88 18.73 $\pm $ 1.18 28.29 $\pm $ 3.59d 0.39 $\pm $ 0.04  
149757 u 40.98 $\pm $ 6.00 25.44 $\pm $ 0.82 29.32 $\pm $ 1.96d 2.68 $\pm $ 0.05 4.40g
151932 u 79.15 $\pm $ 9.88 26.76 $\pm $ 3.42 15.13 $\pm $ 3.38 2.43 $\pm $ 0.07  
152270 u 56.54 $\pm $ 12.81 17.79 $\pm $ 2.61 25.10 $\pm $ 1.14 1.59 $\pm $ 0.10  
154368 u 169.84 $\pm $ 15.73 61.75 $\pm $ 4.10 21.46 $\pm $ 1.67 26.44 $\pm $ 2.07e 14.45h
154811 u 51.90 $\pm $ 9.15 22.85 $\pm $ 2.79 39.43 $\pm $ 2.59d 0.17 $\pm $ 0.04  
163800 h/u 78.43 $\pm $ 14.27 34.36 $\pm $ 2.16 16.02 $\pm $ 0.86 2.96 $\pm $ 0.08  
164794 u 32.26 $\pm $ 11.89 11.86 $\pm $ 2.47 10.32 $\pm $ 0.72 0.27 $\pm $ 0.06  
169454 u 98.76 $\pm $ 13.17 42.90 $\pm $ 2.79 19.50 $\pm $ 1.42 40.22 $\pm $ 2.38e  
We designate data from the literature as follows: a - Roueff (1996); b - Felenbok & Roueff (1996); c - Boissé et al. (2005). To avoid saturation effects in the case of CH+ and CN molecules we used the unsaturated: d - CH+ A-X (1, 0) line at 3957 Å; $d^{\prime}$ - CH+ A-X (2, 0) line at 3745 Å; e - CN B-X (1, 0) band at 3579 Å; f - CN A-X (1, 0) band at 9186 Å. Data on H2 taken from g - Savage et al. (1977); h - Rachford et al. (2002); c - Boissé et al. (2005).

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