Laboratory Measurements of Fe XXIV L-Shell Line Emission

Details Laboratory Measurements of Fe XXIV L-Shell Line Emission Laboratory Measurements of Fe XXIV L-Shell Line Emission

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...470l..73s&link_type=abstract

Astrophysical Journal Letters v.470, p.L73

Astronomy and Astrophysics

Astronomy

20

Atomic Data, Atomic Processes, Methods: Laboratory, X-Rays: General

Scientific paper

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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