Published June 1991
| Version v1
Journal article
Calculations concerning the reaction C + H3(+) - CH(+) + H2
Creators
- 1. Duke University, Durham, NC (USA)
- 2. IBM Almaden Research Center, San Jose, CA (USA)
- 3. Molecular Research Institute, Palo Alto (USA)
- 4. Laboratoire de Radioastronomie Millimetrique, Paris (France)
- 5. Molecular Research Institute, Palo Alto, CA (USA)
Description
The ion-molecule reaction of C + H3(+) - CH(+) + H2 has not been studied in the laboratory but is thought to be important in the gas phase synthesis of organic molecules in dense interstellar clouds. This reaction was studied theoretically by performing quantum chemical ab initio calculations on the potential surface. It is found that there is no activation barrier to the reaction and that it proceeds smoothly to the first excited electronic state of CH(+). The rate coefficient as a function of temperature can then be estimated using the proper long-range potentials. The rate coefficient at 10 K is calculated to be 2.9 x 10 to the -9th cu cm/sec. 18 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 374
- Series
- Astrophys. J.
- Journal Page Range
- 390-393
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22078950
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHEMICAL COMPOSITION; COSMIC GASES; COSMOCHEMISTRY; HYDROCARBONS; INTERSTELLAR SPACE; MOLECULAR STRUCTURE; ORGANIC COMPOUNDS; SYNTHESIS
- Descriptors DEC
- CHEMISTRY; FLUIDS; GASES; SPACE