Airborne Observations of the H 18 20 2 21 2 12 Transition in the Shocked Region of Orion BN-IRc2

Astronomy and Astrophysics – Astronomy

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Ism: Abundances, Ism: Molecules, Ism: Individual Alphanumeric: Irc2, Ism: Jets And Outflows

Scientific paper

We report the first far-IR detection of isotopic water in the Orion BN-IRc2 region from aboard the Kuiper Airborne Observatory. The observation of the 183.5290 mu m H218O 221 --> 212 emission line indicates that it is likely to originate from shocked gas in the outflow around Orion BN-IRc2, rather than from warm gas of the Orion plateau, where the H2O abundance is low ([H2O]/[H] <~ 2.5 x 10-5). Our observation infers a ratio of [H2O]/[H] <~ 1.7 x 10-3, which indicates that O is efficiently converted to H2O in shocked gas.

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