The CN red system in the solar spectrum

Details The CN red system in the solar spectrum The CN red system in the solar spectrum

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...259..381s&link_type=abstract

Astrophysical Journal, Part 1, vol. 259, Aug. 1, 1982, p. 381-391. Research supported by the Robert A. Welch Foundation, Univer

Astronomy and Astrophysics

Astrophysics

64

Cn Emission, Line Spectra, Molecular Spectra, Solar Spectra, Cool Stars, Oscillators, Photosphere, Radiative Lifetime, Spectral Bands, Transition Probabilities

Scientific paper

Solar CN lines from leading bands of the Delta-v = -2, -1, 0, +1, +2, and +3 sequences of the A 2Pi-X 2 Sigma(+) red system are analyzed to provide band absorption oscillator strengths, radiative lifetimes of the A 2Pi state and the electronic transition moment. The results are compared with recent experimental results and an ab initio calculation. In general, the solar analysis is consistent with both the experiments and the ab initio predictions. Additional experiments are called for in order to resolve one outstanding discrepancy and to provide accurate oscillator strengths for the infrared (Delta-v is less than or equal to -1) sequences which are potentially key bands in the analysis of spectra of cool stars.

Affiliated with

Also associated with

No associations

Rating

The CN red system in the solar spectrum 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 The CN red system in the solar spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The CN red system in the solar spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-899715