Published July 15, 1975
| Version v1
Journal article
A comparative study of H2CO, OH, and H I in the dark Taurus dust cloud
Description
High-sensitivity spectra of H2CO, OH, and H I, all taken with the same angular resolution, were obtained in the dark dust cloud in Taurus. At some positions there exist three velocity components, instead of the two revealed by previous investigations. H I correlates rather well, but not perfectly, with the molecules, suggesting that much of it resides outside the region containing the molecules
Additional details
Identifiers
- DOI
- 10.1086/153698;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 199
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 361
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 7226581
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHEMICAL COMPOSITION; COSMIC DUST; FORMALDEHYDE; HYDROGEN; HYDROXYL RADICALS; INTERSTELLAR SPACE; MOLECULES; NEBULAE; RADIOWAVE RADIATION; SPECTRA; TEMPERATURE DEPENDENCE; VARIATIONS; VELOCITY
- Descriptors DEC
- ALDEHYDES; DUSTS; ELECTROMAGNETIC RADIATION; ELEMENTS; NONMETALS; ORGANIC COMPOUNDS; RADIATIONS; RADICALS; SPACE
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent