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Table 3

Chemical models.

Model A V n H a T K T dust ζ(H2) b Metallicityc
(mag) (cm-3) (K) (K) (s-1)

Diffused 0.5 70 100 17 2 × 10-16 High
Translucentd 3 5 × 103 30 & 50 10 1.3 × 10-17 Low
Densed 10 2 × 104 10 & 30 10 1.3 × 10-17 Low
Sgr B2 (M) envelopee 300 4 × 103 40 10 4× 10-16 High

Notes. All models use a ultraviolet flux of 1 G0.

(a)

The total hydrogen density nH = 2n(H2) + n(H).

(b)

The cosmic ionisation rate of molecular hydrogen (cf. Indriolo et al. 2012).

(c)

The assumed initial metal abundances are found in Table D.5.

(d)

Typical conditions in respective cloud type (e.g. Snow & McCall 2006).

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