Laboratory Evidence for Efficient Water Formation in Interstellar Ices
Even though water is the main constituent in interstellar icy mantles, its chemical origin is not well understood. Three different formation routes have been proposed following hydrogenation of O, O sub(2), or O sub(3) on icy grains, but experimental evidence is largely lacking. We present a solid s...
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Veröffentlicht in: | The Astrophysical journal 2008-10, Vol.686 (2), p.1474-1479 |
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Sprache: | eng |
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