| Autor: |
Dorodnitsyn, A., Kallman, T. |
| Předmět: |
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| Zdroj: |
AIP Conference Proceedings; 10/1/2009, Vol. 1171 Issue 1, p304-308, 5p, 3 Graphs |
| Abstrakt: |
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. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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