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- W56501853 abstract "The first astronomical detections of the (J, K)=(10, 10), (11, 11), (12, 12), (13, 13) and (14, 14) doublet inversion emission lines of NH 3 at 1 cm wavelength are presented. These transitions are emitted from energy levels up to 1900 K above the ground state; these are the most energetic states probed by quasithermal radio emission lines. The linewidths and radial velocities are consistent with emission from the Hot Core of the Orion KL nebula. There is no systematic change in ΔV 1/2 and V lsr with (J, K). The spectra also show no wide linewings; these findings agree with results for inversion transitions between lower lying doublet levels" @default.
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- W56501853 date "1993-09-01" @default.
- W56501853 modified "2023-09-27" @default.
- W56501853 title "Hot ammonia emission : kinetic temperature gradients in Orion-KL." @default.
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