Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.2709p&link_type=abstract
American Astronomical Society Meeting 205, #27.09; Bulletin of the American Astronomical Society, Vol. 36, p.1389
Astronomy and Astrophysics
Astronomy
Scientific paper
We compute and apply high precision atomic data from the Iron/RmaX Projects to numerical simulations of (A) the broad line region spectra of Fe I/II/III/IV from the prototypical NLyS1 galaxy I Zw 1, and (B) monochromatic X-ray opacities of the warm absorber in AGN. Ongoing work is part of two projects: The Iron Project that focuses on Fe-peak elements, and the RmaX Project aimed at spectral diagnostics of X-ray plasmas. The primary atomic processes include electron impact excitation, photoionization, (electron-ion) recombination, and spectral transitions. We demonstrate time-dependent spectral diagnostics of the 6.7 keV complex of He-like Fe XXV under transient conditions possible in flares and observable from Astro-2E. We compare the close coupling R-matrix data with the Distorted Wave approximation and the effect on X-ray spectral analysis. We describe the electronic database TIPTOPbase, which will also make available new stellar opacities and radiative accelerations from the Opacity Project.
Nahar Sultana N.
Pradhan Anil Kumar
Rodriguez-Ardila Alberto
Sigut Thomas Allan Aaron
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