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- W2004106315 abstract "A large number of previously unreported molecular transitions have been detected in the submillimeter wavelength band toward OMC-1 and M17 SW using the Texas 4.9 m radio antenna. The emission components in OMC-1 that come from the unresolved plateau and hot core regions are stronger in these higher energy transitions than in the lower-energy, lower-frequency lines. Intense, probably thermalized high J SiO lines require a very hot core if they arise in a region the same size as that mapped in J = 2-1 SiO by interferometer measurements. Despite the high energy levels of the submillimeter lines of CN and CCH, there is no broad emission component evident, consistent with their greatly reduced abundance due to removal by chemical reactions. 33 references." @default.
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- W2004106315 date "1986-11-01" @default.
- W2004106315 modified "2023-09-27" @default.
- W2004106315 title "Submillimeter molecular spectroscopy with the Texas millimeter wave observatory radio telescope" @default.
- W2004106315 doi "https://doi.org/10.1086/164741" @default.
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