Published June 1986 | Version v1
Journal article

Microwave and far-infrared spectra of the O-(18)H radical

  • 1. NBS, Boulder, CO
  • 2. Arizona State Univ., Tempe
  • 3. Oxford Univ., England

Description

Far-infrared laser magnetic resonance (LMR) spectroscopy was used to calculate the frequencies, wavelengths, and line strengths for transitions of O-(18)H molecules at microwave and far-infrared frequencies. In this experiment, a molecular transition frequency is tuned into coincidence with that of a fixed frequency laser by the application of a variable magnetic field. The O-(18)H radicals, detected in natural abundance (0.20 percent), were produced by the reaction of hydrogen atoms with nitrogen dioxide. These data together with microwave frequencies ascertained by Gottlieb, Redford, and Smith (1974) were used to determine the parameters of an effective Hamiltonian. Rotational levels up to J = 5.5 were involved. Results are indicated schematically and the low-lying energy levels of O-(18)H are shown. It is concluded that the frequencies of transitions between levels studied directly in the LMR experiment are reliable. 18 references

Additional details

Publishing Information

Journal Title
Astrophys. J.
Journal Volume
305
Series
Astrophys. J.
Journal Page Range
513-517
ISSN
0004-637X
CODEN
ASJOA