Modeling the FeK line profiles in type i active galactic nuclei with a compton-thick disk wind
We have modeled a small sample of Seyfert galaxies that were previously identified as having simple X-ray spectra with little intrinsic absorption. The sources in this sample all contain moderately broad components of FeK-shell emission and are ideal candidates for testing the applicability of a Compton-thick accretion disk wind model to active galactic nucleus (AGN) emission components. Viewing angles through the wind allow the observer to see the absorption signature of the gas, whereas...[Show more]
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|Source:||Astrophysical Journal, The|
|01_Tatum_Modeling_the_FeK_line_profiles_2012.pdf||728.31 kB||Adobe PDF||Request a copy|
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