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- W2034954259 abstract "Rotationally excited carbon monoxide has been detected in the Galactic H II region/molecular cloud complex G333.6–0.2 in the 163-µm J = 16→15 and 186-µm J = 14→13 transitions. These detections, together with an upper limit to the J = 21→20 transition at 124 µm indicate that the excited CO emission comes from gas of kinetic temperature 200 to 800 K and pressure ≈ 5 × l07 K cm−3. A high-resolution spectrum of the J = 14→13 transition shows CO emission over more than 80 km s−1, possibly with a double peaked profile centred near the systemic velocity of G333.6–0.2. The far-infrared CO emission probably comes from shocked gas (mass ≈ 30 |$M_odot$|) in mass outflow from newly formed, massive stars. The detection of the J = 14→13 transition is the first to be made of this line in any source, and is the longest wavelength line yet detected in interstellar space by non-heterodyne techniques." @default.
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- W2034954259 date "1989-04-01" @default.
- W2034954259 modified "2023-09-23" @default.
- W2034954259 title "Shocked carbon monoxide in G333.6-0.2" @default.
- W2034954259 doi "https://doi.org/10.1093/mnras/237.4.1001" @default.
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