Photoionization Modeling: the K Lines and Edges of Iron

Details Photoionization Modeling: the K Lines and Edges of Iron Photoionization Modeling: the K Lines and Edges of Iron

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..774...75p&link_type=abstract

X-RAY DIAGNOSTICS OF ASTROPHYSICAL PLASMAS: Theory, Experiment, and Observation. AIP Conference Proceedings, Volume 774, pp. 75

Astronomy and Astrophysics

Astrophysics

Photoionisation, X-Ray Spectroscopy, Atomic And Molecular Data, Spectra, And Spectral Parameters, Atomic Processes And Interactions, Photoionization Of Atoms And Ions, X-Ray

Scientific paper

We calculate the efficiency of iron K line emission and iron K absorption in photoionized models using a new set of atomic data. These data are more comprehensive than those previously applied to the modeling of iron K lines and edges from photoionized gases, and allow us to systematically examine the behavior of the properties of line emission and absorption as a function of the ionization parameter, density and column density of model constant density clouds.

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