Dissociative recombination of H3+ and some other interstellar ions: a controversy resolved
- 30 November 1993
- journal article
- Published by Elsevier in International Journal of Mass Spectrometry and Ion Processes
- Vol. 129, 163-182
- https://doi.org/10.1016/0168-1176(93)87040-y
Abstract
No abstract availableKeywords
This publication has 32 references indexed in Scilit:
- The ion chemistry of interstellar cloudsChemical Reviews, 1992
- Further measurements of the H+3(v=0,1,2) dissociative recombination rate coefficientThe Journal of Chemical Physics, 1992
- The dissociative recombination rate coefficients of H+3, HN+2, and HCO+The Journal of Chemical Physics, 1990
- H3+ in the Jovian ionosphereJournal of Geophysical Research, 1987
- Low-temperature dissociative recombination of E + H3(+)The Astrophysical Journal, 1984
- Measurements of dissociative recombination coefficients of H+3, HCO+, N2H+, and CH+5 at 95 and 300 K using the FALP apparatusThe Journal of Chemical Physics, 1984
- Energy Dependence of Dissociative Recombination below 0.08 eV Measured with (Electron-Ion) Merged-Beam TechniquePhysical Review Letters, 1979
- Measurements of Recombination of Electrons withandIonsPhysical Review A, 1973
- Dissociative RecomibnationPublished by Elsevier ,1970
- Electron Loss Process in the Hydrogen AfterglowPhysical Review B, 1955