The formation of narrow X-ray line spectra from realistic hydrodynamical models: applications to the problem of warm absorbers

Details The formation of narrow X-ray line spectra from realistic hydrodynamical models: applications to the problem of warm absorbers The formation of narrow X-ray line spectra from realistic hydrodynamical models: applications to the problem of warm absorbers

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1171..304d&link_type=abstract

RECENT DIRECTIONS IN ASTROPHYSICAL QUANTITATIVE SPECTROSCOPY AND RADIATION HYDRODYNAMICS: Proceedings of the International Confe

Astronomy and Astrophysics

Astrophysics

Radiative Transfer, X-Ray Spectra, Galactic Nuclei, Radiative Transfer, Scattering, Acoustic Cavitation In Liquids, Galactic Center, Bar, Circumnuclear Matter, And Bulge

Scientific paper

We calculate a series of synthetic spectra from outflows originating from the obscuring torus in active galactic nuclei (AGN). Such modeling includes 2.5D hydrodynamical simulations of an X-ray excited torus wind, including the effects of X-ray heating, ionization, and radiation pressure. 3D radiation transfer calculations are performed in the 3D Sobolev approximation. Synthetic X-ray line spectra and individual profiles of several strong lines are shown at different inclination angles, observing times, and for different characteristics of the torus.

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