NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Calculations concerning the reaction C + H3(+) - CH(+) + H2The 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.
Document ID
19910055392
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Talbi, D.
(Molecular Research Institute, Palo Alto, CA; Laboratoire de Radioastronomie Millimetrique Paris, France)
Defrees, D. J.
(Molecular Research Institute, Palo Alto; IBM Almaden Research Center San Jose, CA, United States)
Egolf, D. A.
(Molecular Research Inst. Palo Alto, CA, United States)
Herbst, Eric
(Duke University Durham, NC, United States)
Date Acquired
August 15, 2013
Publication Date
June 10, 1991
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 374
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
91A40015
Funding Number(s)
CONTRACT_GRANT: NAG2-16
CONTRACT_GRANT: NSF AST-89-15190
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available