Photoionization Modeling: the K Lines and Edges of
Iron
Dr. Patrick Palmeri, T.R. Kallman, C. Mendoza,
M.A. Bautista, J. Krolik
Astrophysique et Spectroscopie  UMH
20 Place du Parc
B7000 Mons, Belgium
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.
