Free Access
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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.