Electron impact excitation of N III - Fine-structure collision strengths and Maxwellian-averaged rate coefficients

Details Electron impact excitation of N III - Fine-structure collision strengths and Maxwellian-averaged rate coefficients Electron impact excitation of N III - Fine-structure collision strengths and Maxwellian-averaged rate coefficients

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.266..715s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 266, p. 715

Astronomy and Astrophysics

Astronomy

17

Nitrogen Ions, Fine Structure, Atomic Spectra, Electron Impact, Solar Spectra, Stellar Spectra, Planetary Nebulae, Chebyshev Approximation, Tables (Data)

Scientific paper

The R-matrix method is used to calculate collision strengths and Maxwellian averaged rate coefficients for some fine-structure transitions in N III. Analytic fits are given for the rate coefficients for the range of temperatures 5000-200,000 K, so that they may be readily applied to solar/late-type star and planetary nebula investigations. The present data have significant differences from earlier calculations.

Affiliated with

Also associated with

No associations

Rating

Electron impact excitation of N III - Fine-structure collision strengths and Maxwellian-averaged rate coefficients does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Electron impact excitation of N III - Fine-structure collision strengths and Maxwellian-averaged rate coefficients, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Electron impact excitation of N III - Fine-structure collision strengths and Maxwellian-averaged rate coefficients will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1017838