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...

সম্পূর্ণ বিবরণ

গ্রন্থ-পঞ্জীর বিবরন
প্রধান লেখক: Tatum, M, Turner, T, Sim, SA, Miller, L, Reeves, J, Patrick, A, Long, K
বিন্যাস: Journal article
ভাষা:English
প্রকাশিত: Institute of Physics Publishing 2012