![]() |
CiteULike | ![]() |
vescalant's CiteULike | ![]() |
![]() |
|
![]() |
Register | ![]() |
Log in | ![]() |
Effective recombination coefficients for N II lines at nebular temperatures and densitiesby: R. Kisielius, P. J. Storey
|
Reviews
[Write a review of this article]
Find related articles from these CiteULike users
Find related articles with these CiteULike tags
Posting History
AbstractWe calculate effective recombination coefficients for the formation of selected lines of N II. New photoionization data are computed which accurately map the near threshold resonances and are used to derive recombination coefficients for principal quantum numbers, $n ≤ 15$, 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.
BibTeX record
RIS record