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Table 2

Results of optical depth fits and resulting o-NH3 abundances derived from H2CO observations by Wadiak et al. (1988) and CH observations by Polehampton et al. (2005b).

Feature τNH3a ΔVNH3 N(o-NH3) N(NH3)mod V LSR,H2CO N(H2CO) X(o-NH3)b VLSR,CHc N(CH) X(o-NH3)d
[km s-1] [cm-2] [cm-2] [km s-1] [cm-2] [km s-1] [cm-2]

 A 0.71 9.8 2.7 × 1013 6.9 × 1013  −105  ~6.1 × 1013e  ~9.0 × 10-10e  −107.6 0.9 × 1014 1.2 × 10-8
B 0.44 12.8 2.2 × 1013 5.5 × 1013  −75  < 2.3 × 1013  > 1.9 × 10-9  −81.7 2.6 × 1014 3.4 × 10-9
C 1.57 4.3 2.7 × 1013 6.6 × 1013  −41 3.3 × 1013 1.6 × 10-9  −44.0 1.5 × 1014 7.1 × 10-9
D I 0.46 3.5 6.2 × 1012 1.6 × 1013  −27  < 7.0 × 1012  > 1.8 × 10-9
D II 0.46 4.4 8.0 × 1012 2.0 × 1013  −20  < 1.2 × 1013  > 1.3 × 10-9  −24.4 1.9 × 1014 1.7 × 10-9
F 0.52 8.5 1.7 × 1013 4.3 × 1013  +32 1.1 × 1013 3.2 × 10-9  +31.4 1.5 × 1014 4.6 × 10-9

Notes. Including total ammonia column densities estimated by the representative RADEX model of a diffuse molecular cloud for comparison.

(a)

Central optical depth ;

(b)

calculated assuming X(H2CO) = [H2CO]/[H2] = 2 × 10-9 (Dickel & Goss 1990);

(c)

velocities from H i absorption data (Garwood & Dickey 1989);

(d)

calculated assuming X(CH) = [CH]/[H2] = 4 × 10-8 (Liszt & Lucas 2002);

(e)

from Downes et al. (1980), assuming Tex = 3.1 K.

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