The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks

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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