Published February 1989
| Version v1
Journal article
Collisional rate coefficients of C3H2 and the determination of physical conditions in molecular clouds
Creators
- 1. NASA, Goddard Institute for Space Studies, New York, NY (USA)
- 2. National Research Council of Canada, Herzberg Institute of Astrophysics, Ottawa
Description
Collisional excitation rates for C3H2, calculated using the coupled states approximation at temperatures of 10-30 K, are presented. C3H2 produces a number of spectral line pairs whose members are close together in frequency but arise from levels with different excitation energies. The rates are used in statistical equilibrium calculations to illustrate the excitation properties and density-dependent behavior of various C3H2 line ratios. 17 references
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 337
- Series
- Astrophys. J.
- Journal Page Range
- 306-317
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20062649
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHEMICAL COMPOSITION; COSMIC GASES; EXCITATION; HYDROCARBONS; INTERSTELLAR SPACE; LOW TEMPERATURE; MOLECULE COLLISIONS; SPECTRA; VERY LOW TEMPERATURE
- Descriptors DEC
- COLLISIONS; ENERGY-LEVEL TRANSITIONS; FLUIDS; GASES; ORGANIC COMPOUNDS; SPACE