MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND

MODELING THE Fe K 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 Com...

Bibliografski detalji
Glavni autori:	Tatum, M, Turner, T, Sim, SA, Miller, L, Reeves, J, Patrick, A, Long, K
Format:	Journal article
Jezik:	English
Izdano:	Institute of Physics Publishing 2012

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