Rate of CH3(+) + H2 yields CH5(+) + HV and role of electronic transitions in other radiative association processes

Details Rate of CH3(+) + H2 yields CH5(+) + HV and role of electronic transitions in other radiative association processes Rate of CH3(+) + H2 yields CH5(+) + HV and role of electronic transitions in other radiative association processes

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...312..363b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 312, Jan. 1, 1987, p. 363-366.

Astronomy and Astrophysics

Astrophysics

26

Cosmochemistry, Electron Transitions, Interstellar Matter, Methane, Molecular Clouds, Reaction Kinetics, Cyclotron Radiation, Radiative Transfer

Scientific paper

A result obtained from a recent reinterpretation of experimental data on CH3++H2 → CH5++hν is used to revise values given earlier for the rate coefficients of this process at 13, 30, and 80K. It is also argued that radiative electronic transitions are responsible for stabilization in many of the ion-molecule association processes of interest in connection with interstellar cloud chemistry.

Affiliated with

Also associated with

No associations

Rating

Rate of CH3(+) + H2 yields CH5(+) + HV and role of electronic transitions in other radiative association processes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Rate of CH3(+) + H2 yields CH5(+) + HV and role of electronic transitions in other radiative association processes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rate of CH3(+) + H2 yields CH5(+) + HV and role of electronic transitions in other radiative association processes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1622255