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Table 1.
Overall reactions adopted for modelling dust accretion in the ISM.
| Species | Reactions | Molecules |
|---|---|---|
| Olivine | 2Mg + SiO + 3H2O → Mg2SiO4(s)+3H2 | Mg, SiO, H2O |
| Pyroxene | Mg + SiO + 2H2O → MgSiO3(s) + 2H2 | Mg, SiO, H2O |
| Fe(s) | Fe→Fe(s) | Fe |
| C(s) | C2H2→2C(s)+H2 | C2H2 |
Notes. The molecules and atoms in the gas phase from which each dust species is formed are also listed.
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