Master Equation Modelling of Non-equilibrium Chemistry in Stellar Outflows

Supplementary Information for a Faraday Discussion paper.

Contents:

Figure S1. Potential energy surface for the reaction between SiO₂ and H₂O. Energies are calculated at the cbs-qb3 level of theory [Montgomery et al., 1999].

Table S1. Molecular properties and heats of formation (at 0 K) of the stationary points on the SiO₂ + H₂O potential energy surface.

Table S2. Reaction scheme for forming gas-phase Ca, Fe and Mg silicate molecules in the stellar outflow.