Model for Astrophysical X-Ray Absorption Fine Structure

Details Model for Astrophysical X-Ray Absorption Fine Structure Model for Astrophysical X-Ray Absorption Fine Structure

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...505..236f&link_type=abstract

The Astrophysical Journal, Volume 505, Issue 1, pp. 236-243.

Astronomy and Astrophysics

Astronomy

8

Ism: Dust, Extinction, Galaxies: Ism, Techniques: Spectroscopic, X-Rays: Galaxies

Scientific paper

We present a theoretical model and database designed to provide analysis of astrophysical X-ray absorption fine structure (XAFS). The model includes spherical wave corrections and multiple-scattering contributions to the modification of the X-ray absorption coefficient. The model and database provide the basis for the astrophysical XAFS analysis (AXA) tool, which may be used to analyze properties of interstellar grains and molecules from high-resolution X-ray spectra expected to be observed by future satellite missions (e.g., the Advanced X-ray Astrophysics Facility).

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