The A 2 S / -X 2 P i near-infrared electronic transition of AgO was observed for the first time. The spectrum was recorded with the high resolution Fourier transform spectrometer associated with the McMath-Pierce Solar Telescope at Kitt Peak. The excited AgO molecules were produced in a low pressure
Fourier-Transform Microwave Spectroscopy of CCN (X2Π1/2)
✍ Scribed by Y. Ohshima; Y. Endo
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 379 KB
- Volume
- 172
- Category
- Article
- ISSN
- 0022-2852
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✦ Synopsis
The lowest (J=\frac{3}{2}-\frac{1}{2}) rotational transition of the (\mathrm{CCN}) radical in its (X^{2} \Pi_{1 / 2}) state has been observed by using a Fabry-Perot-type Fourier-transform microwave spectrometer combined with a pulsed discharge nozzle. The radical has been generated by a pulsed electric discharge of (\mathrm{CH}{3} \mathrm{CN}) or (\mathrm{CCl}{3} \mathrm{CN}) diluted in (\mathrm{Ar}), and subsequently cooled to a few degrees in a supersonic free jet. The spectrum with completely resolved fine and hyperfine structures has been analyzed to provide an accurate set of spectroscopic constants. The spin density and other electronic properties of the unpaired electron in the radical have been estimated from the determined hyperfine coupling constants associated with the nitrogen nucleus. (C) 1995 Academic Press. Inc
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