Atomic Physics Calculations for Iron L-Line Spectra

Details Atomic Physics Calculations for Iron L-Line Spectra Atomic Physics Calculations for Iron L-Line Spectra

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..627d&link_type=abstract

Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 July

Astronomy and Astrophysics

Astronomy

Scientific paper

Absorption spectra of iron L-lines are observed in AGN by Chandra and XMM-Newton. FeXXIV to Fe XVII lines corespond to transitions between ground and excited levels whereas Fe XVI to Fe VII lines involve autoionizing levels as upper levels. Theoretical atomic data for n=2-3 and n=2-4 radiative transitions will be presented : wavelengths radiative and autoionization probability rates. We shall also discuss their applications to the photoionized plasmas in Seyfert galaxies.

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