Atomic data for the X-ray lines of iron.

Details Atomic data for the X-ray lines of iron. Atomic data for the X-ray lines of iron.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..671b&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 671 - 672

Astronomy and Astrophysics

Astrophysics

Atomic Data: Iron Lines, Iron: X-Ray Lines, Photoionization: Atomic Data

Scientific paper

Iron is an astrophysically abundant element, and the X-ray lines of iron and its ions (especially the K lines in some cases) are important sources of information on the structure of and processes in and around certain astronomical objects. To interpret these lines one needs accurate atomic data about the atoms and ions from which they arise: photoionisation cross-sections are one of the most important sources of such information. This paper presents the results of R-matrix calculations on the photoionisation cross-section of Fe XXIV (total, 1s photoejection and partial cross-sections), which is the start of a series of such calculations on the ions of iron.

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