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- W117004849 abstract "Various models of water maser emission in star forming regions, based both on collisional and 6.3 gm radiative pumping mechanisms, require appreciable rates of excitation of water into its first vibrationally excited bending mode. We report the detection in Orion, using the 12-meter NRAO radiotelescope at Kitt Peak, of a line coincident in frequency with the 414 →321 rotational transition of the ν2 vibrational manifold of ortho-H2O at vLSR ~18 km s-1. If the detected line is indeed due to this water transition, a beam-averaged column density of ~1013 cm-2 in the vibrationally excited upper level is implied.KeywordsColumn DensityRotational TransitionWater TransitionNASA Goddard SpaceAppreciable RateThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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- W117004849 date "1990-01-01" @default.
- W117004849 modified "2023-09-27" @default.
- W117004849 title "Vibrationally Excited H2O in Orion A" @default.
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- W117004849 doi "https://doi.org/10.1007/978-94-015-6850-0_104" @default.
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