Effective recombination coefficients for lines at nebular temperatures and densities *
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
2 Institute of Theoretical Physics and Astronomy, A. Goštauto 12, Vilnius, LT-2600, Lithuania
Corresponding author: P. J. Storey, email@example.com
Accepted: 18 February 2002
We calculate effective recombination coefficients for the formation of selected lines of . New photoionization data are computed which accurately map the near threshold resonances and are used to derive recombination coefficients for principal quantum numbers, , including radiative and dielectronic recombination. Cascading from higher states is included, allowing for the effects of finite electron density in a hydrogenic approximation. The effects of population in the excited states of the recombining ion are investigated.
Key words: atomic data / line: formation / ISM: HII regions / planetary nebulae: general
© ESO, 2002