Electron Impact Excitation of NII - Fine Structure Collision Strengths and Maxwellian-Averaged Rate Coefficients

Details Electron Impact Excitation of NII - Fine Structure Collision Strengths and Maxwellian-Averaged Rate Coefficients Electron Impact Excitation of NII - Fine Structure Collision Strengths and Maxwellian-Averaged Rate Coefficients

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.268..816s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 268, NO. 3/JUN1, P. 816, 1994

Astronomy and Astrophysics

Astronomy

39

Atomic Processes - Line: Formation - Sun: Chromosphere - Stars: Late-Type - Planetary Nebulae: General

Scientific paper

An elaborate 13-state R-matrix calculation is performed to determine collision strengths and Maxwellian-averaged rate coefficients for fine-structure transitions in N II. Analytic fits are given for the rate coefficients for the temperature range 5000-125 892 K, so that they may be applied to investigations of solar/late-type stars and planetary nebulae.

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