EDP Sciences
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Free Access
Issue
A&A
Volume 503, Number 2, August IV 2009
Page(s) 323 - 343
Section Astrophysical processes
DOI https://doi.org/10.1051/0004-6361/200912129
Published online 22 June 2009

Online Material

Table 6:   As Table 5, for $b({{\rm CO}})=0.3$ km s-1, $T_{{\rm ex}}({{\rm CO}})=50$ K and $N(^{12}{{\rm CO}})/N(^{13}{{\rm CO}})=69$a.

Table 7:   As Table 5, for $b({{\rm CO}})=3.0$ km s-1, $T_{{\rm ex}}({{\rm CO}})=5$ K and $N(^{12}{{\rm CO}})/N(^{13}{{\rm CO}})=69$a.

Table 8:   As Table 5, for $b({{\rm CO}})=0.3$ km s-1, $T_{{\rm ex}}({{\rm CO}})=5$ K and $N(^{12}{{\rm CO}})/N(^{13}{{\rm CO}})=35$a.

Table 9:   Elemental abundances.

Table 10:   Column densities (in cm-2) for our grid of translucent cloud models at $T_{{\rm gas}}=15$ K. Results for $n_{{\rm H}}=500$ and 700 cm-3 are not shown.

Table 11:   As Table 10, for $T_{{\rm gas}}=30$ K.

Table 12:   As Table 10, for $T_{{\rm gas}}=50$ K.

Table 13:   As Table 10, for $T_{{\rm gas}}=100$ K.


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