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On the nucleation of dust in oxygen-rich stellar outflows

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Figure

Table 1. Properties of the Ca, Mg and Fe titanate and silicate molecules
Table 2. Reaction scheme for forming gas-phase Ca, Fe and Mg titanate and silicate molecules in the stellar outflow
Table 3. Molecular properties and relative energies of the stationary points on the potential energy surface for Ca + OTi(OH)2  CaTiO3 + H2
Table 4. Energies of the stationary points on the potential energy surfaces of Ca, Fe and Mg with OSi(OH)2, relative to the reactants (Mt = Ca, Fe or Mg)
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