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- W2089784200 abstract "In previous work (Morgenthaler et al. and Glinski et al.), we proposed a revision to the standard OH photochemistry of van Dishoeck & Dalgarno in order to explain the anomalously bright [O I] 6300 Å emission observed by several instruments in comet C/1995 O1 (Hale-Bopp). In order to test the validity of revisions to the OH photochemistry, we present wide-field Fabry-Pérot [O I] 6300 Å observations of comet C/1996 B2 (Hyakutake) and review similar observations recorded for 1P/Halley and 1989 c1 (Austin). Conventional long-slit spectroscopic observations of several comets in [O I] are also reviewed. The bulk of the evidence suggests that the OH photochemical rates of van Dishoeck & Dalgarno are, on the whole, correct and that the bright [O I] emission observed in Hale-Bopp, particularly at cometocentric distances beyond ~3 × 104 km, was unique to that comet, or possibly any comet with such a large production rate." @default.
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- W2089784200 date "2007-03-10" @default.
- W2089784200 modified "2023-09-24" @default.
- W2089784200 title "Large Aperture O<scp>i</scp>6300 A Observations of Comet Hyakutake: Implications for the Photochemistry of OH and O<scp>i</scp>Production in Comet Hale‐Bopp" @default.
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- W2089784200 doi "https://doi.org/10.1086/511062" @default.
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