Published May 1986
| Version v1
Journal article
Detection of the OH Zeeman effect toward Orion A
- 1. Kentucky Univ., Lexington
- 2. Paris Observatoire, Meudon, France
- 3. Illinois Univ., Urbana
Description
The Zeeman effect in the 18 cm OH absorption spectrum of Orion A is detected. From this effect, a line-of-sight magnetic field strength of - 125 + or - 20 is derived. At the same position, an H I Zeeman effect equivalent to a magnetic field of - 49 + or - 4 micro-G is found. Thus, the magnetic field in the molecular gas toward Orion A is significantly stronger than that in the atomic gas, contrary to the recent determination for the Cas A line of sight. Densities in the atomic and molecular regions toward Orion A are estimated and it is found that for this region the data are consistent with B proportional to n exp kappa, kappa = 0.3. 23 references
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 304
- Series
- Astrophys. J.
- Journal Page Range
- L57-L60
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18007403
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION SPECTRA; COSMIC GASES; HYDROXYL RADICALS; H2 REGIONS; INTERSTELLAR MAGNETIC FIELDS; ZEEMAN EFFECT
- Descriptors DEC
- COSMIC RADIO SOURCES; FLUIDS; GASES; MAGNETIC FIELDS; RADICALS; SPECTRA