2000
DOI: 10.1016/s0009-2614(00)01276-8
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2+1 resonance-enhanced multiphoton ionisation spectroscopy of the high ν2 levels of the B̃1E″ Rydberg state of NH3(ND3)

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Cited by 8 publications
(13 citation statements)
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“…10 Cheung et al 11 noted that the 35 observed NH 3 emission intensities from interstellar sources do not correspond to a single rotational temperature. In addition, the inversion transition was detected for the rotational level j k = 11 9 , 12 which should not be populated at interstellar temperatures of 10-300 K, and the j k = 3 3 inversion transition has been predicted 13 40 and observed 14 to exhibit maser activity. These observations clearly showed that the emitting NH 3 is not in thermal equilibrium with its environment.…”
Section: Introductionmentioning
confidence: 91%
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“…10 Cheung et al 11 noted that the 35 observed NH 3 emission intensities from interstellar sources do not correspond to a single rotational temperature. In addition, the inversion transition was detected for the rotational level j k = 11 9 , 12 which should not be populated at interstellar temperatures of 10-300 K, and the j k = 3 3 inversion transition has been predicted 13 40 and observed 14 to exhibit maser activity. These observations clearly showed that the emitting NH 3 is not in thermal equilibrium with its environment.…”
Section: Introductionmentioning
confidence: 91%
“…[39][40][41] One consequence of symmetry and nuclear spin constraints is that only transitions originating from the lower (+) inversion component of the ground state appear in bands in which the final ߥ ଶ is even, whereas only transitions from the upper (−) inversion 35 component appear in bands with final ߥ ଶ odd. Therefore, two vibrational transitions must be excited to probe all individual rotational states.…”
Section: B Rotational Levels and Initial State Selection Of Ndmentioning
confidence: 99%
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