Published June 15, 1980
| Version v1
Journal article
Oscillator strengths for lines of the (0,0) and (1,0) bands of the C 1Pi--X 1Σ+ system of HCl and the abundance of HCl in diffuse interstellar clouds
- 1. Harvard-Smithsonian Center for Astrophysics
Description
Oscillator strengths (f-values) for twenty lines of the (0, 0) band and one line of the (1, 0) band of the C 1Pi--X 1Σ+ system of HCl have been measured using quantitative photographic techniques. The f-value for the R(0) line of the (0, 0) band at 129.0257 nm, which is the stronger of the two lines that have been searched for but not detected in diffuse interstellar clouds, is 0.185 +- 0.037. This value and the observations of absorption by chlorine species in the zeta Oph cloud have been used to reassess aspects of the chemical models of diffuse clouds
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 238
- Journal Issue
- 3
- Series
- Astrophys. J.
- Journal Page Range
- 874-880
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 12579625
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION SPECTRA; CHEMICAL COMPOSITION; CHEMICAL REACTIONS; COSMIC GASES; COSMOCHEMISTRY; ENERGY LEVELS; ENERGY-LEVEL TRANSITIONS; HYDROCHLORIC ACID; INTERSTELLAR SPACE; LINE WIDTHS; MOLECULES; OSCILLATOR STRENGTHS; QUANTITY RATIO; ROTATIONAL STATES; SPECTRAL FUNCTIONS
- Descriptors DEC
- CHEMISTRY; CHLORINE COMPOUNDS; EXCITED STATES; FLUIDS; FUNCTIONS; GASES; HALOGEN COMPOUNDS; HYDROGEN COMPOUNDS; INORGANIC ACIDS; SPACE; SPECTRA