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Table D.1

Initial fractional abundances used in Astrochem, relative to H2.

Species Frac. abun. Frac. abun. Frac. abun. Frac. abun. Remark/Reference
IRAS4B IRAS4A L1448C L1157

H2 1.00 × 100 1.00 × 100 1.00 × 100 1.00 × 100
He 1.70 × 10-1 1.70 × 10-1 1.70 × 10-1 1.70 × 10-1 Asplund et al. (2009)
S+ 1.60 × 10-7 1.60 × 10-7 1.60 × 10-7 1.60 × 10-7 Wakelam & Herbst (2008)
Si+ 1.60 × 10-8 1.60 × 10-8 1.60 × 10-8 1.60 × 10-8 Wakelam & Herbst (2008)
Fe+ 6.00 × 10-9 6.00 × 10-9 6.00 × 10-9 6.00 × 10-9 Wakelam & Herbst (2008)
Na+ 4.00 × 10-9 4.00 × 10-9 4.00 × 10-9 4.00 × 10-9 Wakelam & Herbst (2008)
Mg+ 1.40 × 10-8 1.40 × 10-8 1.40 × 10-8 1.40 × 10-8 Wakelam & Herbst (2008)
e 2.00 × 10-7 2.00 × 10-7 2.00 × 10-7 2.00 × 10-7
NH3(ice) 4.28 × 10-6 4.28 × 10-6 4.28 × 10-6 4.28 × 10-6 10% of all N, Wakelam & Herbst (2008)
CO(ice) 1.70 × 10-5 8.80 × 10-6 9.60 × 10-6 2.80 × 10-5 free parameter to match observed intensity
N2(ice) 4.80 × 10-7 3.00 × 10-7 4.60 × 10-7 9.40 × 10-7 free parameter to match observed intensity
CH3OH(ice) 1.00 × 10-5 3.60 × 10-6 5.00 × 10-6 <2.00 × 10-6 free parameter to match observed intensity
H2O(ice) 2.96 × 10-4 3.08 × 10-4 3.10 × 10-4 2.96 × 10-4 all remaining O, Hincelin et al. (2011)

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