Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...460l..65t&link_type=abstract
Astrophysical Journal Letters v.460, p.L65
Astronomy and Astrophysics
Astronomy
6
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.
Geis Norbert
Nikola Thomas
Poglitsch Albrecht
Timmermann Ralf
No associations
LandOfFree
Airborne Observations of the H 18 20 2 21 2 12 Transition in the Shocked Region of Orion BN-IRc2 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Airborne Observations of the H 18 20 2 21 2 12 Transition in the Shocked Region of Orion BN-IRc2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Airborne Observations of the H 18 20 2 21 2 12 Transition in the Shocked Region of Orion BN-IRc2 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1645091