Recombination coefficients for O II lines at nebular temperatures and densities

Details Recombination coefficients for O II lines at nebular temperatures and densities Recombination coefficients for O II lines at nebular temperatures and densities

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...282..999s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 3, p. 999-1013

Astronomy and Astrophysics

Astrophysics

85

Atomic Spectra, Coefficients, Electron Recombination, H Ii Regions, Line Spectra, Oxygen Spectra, Photoionization, Planetary Nebulae, Radiative Recombination, Configuration Interaction, Electron Density (Concentration), Electron Energy, Electron Orbitals

Scientific paper

Rate coefficients are calculated for the formation of O II lines by recombination. Photoionization data from the Opacity Project are used to calculate recombination coefficients for principal quantum numbers, n less than or = 10, including radiative and dielectronic recombination. Cascading from higher states is included, allowing for the effects of finite electron density in a hydrogenic approximation.

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