Microwave and far-infrared spectra of the O-(18)H radical
Creators
- 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
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18011747
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- CHEMICAL COMPOSITION; ELECTRIC DIPOLES; ENERGY LEVELS; FAR INFRARED RADIATION; HYDROXYL RADICALS; INFRARED SPECTRA; INTERSTELLAR SPACE; MICROWAVE SPECTRA; QUANTUM NUMBERS
- Descriptors DEC
- DIPOLES; ELECTROMAGNETIC RADIATION; INFRARED RADIATION; MULTIPOLES; RADIATIONS; RADICALS; SPACE; SPECTRA