1996 Articles
Laboratory Measurements of Fe XXIV L-Shell Line Emission
Recent ASCA spectra exhibit discrepancies with the relative line intensities of various Fe XXIII and XXIV L-shell emission lines predicted by standard plasma emission codes. To address this issue, we have carried out a series of high-resolution, broadband measurements of Fe XXIV line emission using an electron beam ion trap facility. X-ray lines produced in the trap are detected and resolved using Bragg crystal spectrometers. We report measurements of 3 → 2 and 4 → 2 transitions, which result primarily from electron impact excitation. Overall, good agreement is found with distorted wave calculations.
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Also Published In
- Title
- The Astrophysical Journal Letters
- DOI
- https://doi.org/10.1086/310300
More About This Work
- Academic Units
- Astronomy and Astrophysics
- Published Here
- March 25, 2013