Modeling the Fe K Line Profiles in Type I Active Galactic Nuclei with a Compton-thick Disk Wind (2012)

First Author: {Tatum}, M.~M. And {Turner}, T.~J. And {Sim}, S.~A. And {Miller}, L. And {Reeves}, J.~N. And {Patrick}, A.~R. And {Long}, K.~S.
Attributed to:  Stellar Astrophysics at Keele funded by STFC

Abstract

No abstract provided

Bibliographic Information

Volume: 752

Parent Publication: \apj

Issue: 1204.2535