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• W2021083610 abstract "The chemistry of the early stages of the evolution of a nova wind is examined. The new models include an extended chemistry and, in the light of current model atmosphere calculations, a careful treatment of the photoreactions. The results indicate that the chemistry may be somewhat richer than previously determined and, contrary to the findings of previous studies, is essentially not photon-dominated. The abundance of species such as CN and CO match observations well and the ratio of their abundances may be a useful density diagnostic. However, except at very early times, CO formation does not saturate; this has important implications for the subsequent dust-formation epoch. In particular it provides theoretical backing for those observations which suggest that carbon-rich and silicate dusts can be formed concurrently." @default.
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• W2021083610 date "2004-02-01" @default.
• W2021083610 modified "2023-09-29" @default.
• W2021083610 title "The early chemical evolution of nova outflows" @default.
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• W2021083610 doi "https://doi.org/10.1111/j.1365-2966.2004.07330.x" @default.
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