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Table A.1

Binding energies, prefactors, and initial abundances (with respect to H) assumed for the species considered in this work and the resulting snowlines around 0.1 and 1.0 M stars (defined as the locations where the gas and ice abundances are equal at t = 0).

Species ν / s−1 Ebind/K Abundance Snowline/au
Ha 1.54 × 1011 450
OHa 3.76 × 1015 5698
CO 4.1 × 1013 910 1.2 × 10−4 13/25
O2 1.3 × 1014 1030 0.85 × 10−4 12/21
CH4 2.5 × 1014 1140 2.3 × 10−6 8.4/16
C2H4 4 × 1015 2200 2.4/4.4
C2H6 6 × 1016 2600 1.9/3.5
C2H2 3 × 1016 2800 1.6/2.8
CO2 1.1 × 1015 2980 2.1 × 10−5 1.1/2.1
CH3OH 5.0 × 1014 4850 2.3 × 10−6 0.37/0.62
H2O 1.3 × 1018 6722 1.1 × 10−4 0.23/0.45

Notes. (a)Only relevant for grain-surface reactions

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