RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES AND DENSITIES.
999 - 1013.
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-equal-to 10, including radiative and dielectronic recombination. Cascading from higher states is included, allowing for the effects of finite electron density in a hydrogenic approximation.
|Title:||RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES AND DENSITIES|
|Keywords:||ATOMIC DATA, H-II REGIONS, PLANETARY NEBULAE, GENERAL, DIELECTRONIC RECOMBINATION, OPACITY CALCULATIONS, HYDROGENIC IONS, ATOMIC DATA, INTENSITIES|
|UCL classification:||UCL > School of BEAMS > Faculty of Maths and Physical Sciences
UCL > School of BEAMS > Faculty of Maths and Physical Sciences > Physics and Astronomy
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