Published October 1972
| Version v1
Journal article
Upper limit on the OH abundance in the intercloud medium
Creators
Description
A search for weak OH emission at 1665 and 1667 MHz was carried out in three high-latitude directions containing no compact clouds of H V or dust. No OH emission was detected down to low limits, and the comparison of our upper limits with the known H I and dust-column densities reinforces the suggestion that OH tends to be concentrated to regions of high dust or gas density.
Additional details
Identifiers
- DOI
- 10.1086/111331;
Publishing Information
- Journal Title
- The Astronomical Journal
- Journal Volume
- 77
- Journal Issue
- 8
- Series
- Astron. J.
- Journal Page Range
- 649
- ISSN
- 0004-6256
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 4049376
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC DUST; GHZ RANGE 01-100; HYDROXYL RADICALS; H1 REGIONS; INTERSTELLAR SPACE; MILKY WAY; RADIOWAVE RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; DUSTS; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; GALAXIES; GHZ RANGE; RADIATIONS; RADICALS; SPACE
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent