Photoionization Equilibrium Modeling of Iron L Line Emission

Details Photoionization Equilibrium Modeling of Iron L Line Emission Photoionization Equilibrium Modeling of Iron L Line Emission

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...465..994k&link_type=abstract

Astrophysical Journal v.465, p.994

Astronomy and Astrophysics

Astronomy

66

Atomic Processes, Line: Formation, X-Rays: Stars

Scientific paper

We present models for the emission spectra of photoionized gases in the intermediate energy (0.5- 10 keV) X-ray region, including a detailed and up-to-date treatment of the atomic physics associated with the iron L shell. We discuss the general properties of iron L shell emission line strengths and recombination continuum emission and compare the strengths of these features with iron K shell emission and with the spectral features produced by other elements in the same energy range.

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