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- W66567734 abstract "We have observed the (4,4) and (5,5) inversion transitions of ammonia towards 16 ultracompact HII regions, known to be strong NH 3 (2,2) emitters. 15 of these were detected in the (4,4) line and 10 were also observed and detected in the (5,5) transition. Our results indicate that emission from hot molecular gas is the rule rather than the exception in such regions. Combining our observations with earlier measurements of the (1,1) and (2,2) lines, we find that the inferred level populations can be fit with a single rotational temperature: only G10.47+0.03A and G31.41+0.31 are clearly inconsistent with a single component model." @default.
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- W66567734 date "1992-03-01" @default.
- W66567734 modified "2023-09-26" @default.
- W66567734 title "Hot ammonia toward ultracompact HII regions" @default.
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