Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..669b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 186, Mar. 1979, p. 669-672. Research supported by the Science Research
Astronomy and Astrophysics
Astronomy
14
Astronomical Spectroscopy, Atomic Excitations, Iron, Line Spectra, Atomic Spectra, Oscillators, Radiative Lifetime, Tables (Data)
Scientific paper
Lifetimes of 12 excited levels of Fe I and branching ratios for radiative deexcitation of these levels are calculated from Oxford oscillator strengths and compared with various experimental measurements. It is found that the differences between the calculated and measured values, and their standard deviations, are rather poor, except for the results of Figger et al. (1975), for which the mean deviation is 0.5% and the standard deviation of the differences is 5.8%. It is concluded that the absorption technique used at Oxford yields the oscillator strengths of excited lines more accurately than do lifetime measurements.
Blackwell D. E.
Shallis M. J.
No associations
LandOfFree
Precision measurement of relative oscillator strengths. VII - Comparison between measured lifetimes of excited Fe I levels and values calculated from precise oscillator strengths 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 Precision measurement of relative oscillator strengths. VII - Comparison between measured lifetimes of excited Fe I levels and values calculated from precise oscillator strengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Precision measurement of relative oscillator strengths. VII - Comparison between measured lifetimes of excited Fe I levels and values calculated from precise oscillator strengths will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1653664