arXiv Analytics

Sign in

arXiv:1409.8142 [astro-ph.SR]AbstractReferencesReviewsResources

Fe I Oscillator Strengths for Transitions from High-lying Even-Parity Levels

E. A. Den Hartog, M. P. Ruffoni, J. E. Lawler, J. C. Pickering, K. Lind, N. R. Brewer

Published 2014-09-29Version 1

New radiative lifetimes, measured to $\pm$ 5 % accuracy, are reported for 31 even-parity levels of Fe I ranging from 45061 cm$^{-1}$ to 56842 cm$^{-1}$. These lifetimes have been measured using single-step and two-step time-resolved laser-induced fluorescence on a slow atomic beam of iron atoms. Branching fractions have been attempted for all of these levels, and completed for 20 levels. This set of levels represents an extension of the collaborative work reported in Ruffoni et al. (2014). The radiative lifetimes combined with the branching fractions yields new oscillator strengths for 203 lines of Fe I. Utilizing a 1D-LTE model of the solar photosphere, spectral syntheses for a subset of these lines which are unblended in the solar spectrum yields a mean iron abundance of <log[{\epsilon}(Fe)]> = 7.45 $\pm$ 0.06.

Comments: 18 pages, 4 tables, 4 figures. Accepted for publication in the Astrophysical Journal Supplement Series
Categories: astro-ph.SR, astro-ph.IM
Related articles: Most relevant | Search more
arXiv:1710.07571 [astro-ph.SR] (Published 2017-10-20)
Fe I oscillator strengths for transitions from high-lying odd-parity levels
arXiv:1403.2183 [astro-ph.SR] (Published 2014-03-10)
Stellar laboratories II. New Zn IV and Zn V oscillator strengths and their validation in the hot white dwarfs G191-B2B and RE0503-289
arXiv:2308.14854 [astro-ph.SR] (Published 2023-08-28)
R-Matrix calculations for opacities.II. Photoionization and oscillator strengths of iron ions FeXVII, FeXVIII and FeXIX