Published September 1, 1980
| Version v1
Journal article
Models of molecular clouds and the abundances of H2CO and HCO+
- 1. and Owens Valley Radio Observatory, California Institute of Technology
- 2. Electrical Engineering Research Laboratory and Department of Astronomy, University of Texas at Austin
Description
Observations of HCO+ and H2CO in a sample of 13 molecular clouds have been analyzed by construction of uniform, spherical cloud models. The total densities and the abundance of HCO+ and H2CO relative to H2 which result from these models fall into two domains: one group of clouds has a low temperature, moderate density, and high abundances; the other group has higher temperature and density, but lower abundances. The factor distinguishing these groups may be depletion onto grains in the denser sources
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 240
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 532-546
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 12597939
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON MONOXIDE; CHEMICAL COMPOSITION; COSMOCHEMISTRY; ENERGY SPECTRA; FORMALDEHYDE; FORMYL RADICALS; INTERSTELLAR SPACE; LINE BROADENING; RADIATION TRANSPORT
- Descriptors DEC
- ACYL RADICALS; ALDEHYDES; CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; CHEMISTRY; ORGANIC COMPOUNDS; OXIDES; OXYGEN COMPOUNDS; RADICALS; SPACE; SPECTRA