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1 Introduction
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2 The model
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3 Results
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4 SiO rotational emission lines
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5 Comparisons with observations
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6 Concluding remarks
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References
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Appendix A: SiO radiative transfer
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Appendix B: Fractions of Fe, Si and Mg sputtered from olivine
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Appendix C: Initial gas-phase abundance of O2
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