Line emission from charge transfer with atomic hydrogen at thermal energies

Details Line emission from charge transfer with atomic hydrogen at thermal energies Line emission from charge transfer with atomic hydrogen at thermal energies

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phrva..28.2137s&link_type=abstract

Physical Review A - General Physics, 3rd Series (ISSN 0556-2791), vol. 28, Oct. 1983, p. 2137-2140.

Physics

General Physics

20

Charge Transfer, Electron Plasma, Hydrogen Atoms, Planetary Nebulae, Plasma Spectra, Emission Spectra, Line Spectra, Oxygen Spectra, Thermal Energy

Scientific paper

A list of emission lines of ions of C,N,O, and Ne which are predicted to appear as a result of low-energy charge transfer and which may be useful as diagnostic probes of the processes and of the physical environments in which they take place is presented. Models of planetary nebulae are constructed which demonstrate that several emission lines of O(2+) are produced preferentially by charge transfer recombination of O(3+) ions in collisions with H atoms, and quantitative estimates of the individual channel charged transfer rate coefficients at temperatures near 1 eV are derived.

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