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Submillimeter observations of OH and CH in M42
The Astrophysical Journal1985Vol. 296, pp. 142–142
Citations Over TimeTop 11% of 1985 papers
Abstract
The authors have detected the 2Π1/2 J = 3/2→1/2 transitions of OH at 163.12 and 163.40 μm and obtained upper limits for the 2Π3/2 J = 3/2→1/2 transitions of CH at 149.09 and 149.39 μm, in observations of the Kleinmann-Low nebula of Orion. All four flux levels lie between 1 and 1.2×10-17W cm-3. Taken together with existing data on molecular hydrogen and CO and recent data on other OH transitions, the results suggest OH emission from postshock regions at temperatures T ≈ 103K and densities nH2 ≈ 7×106cm-3 and nOH ≈ 80 cm-3. The OH column density is NOH ≈ 4×1016cm-2 in the emitting regions.
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