MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND (2012)

First Author: Tatum M

Attributed to: Stellar Astrophysics at Keele funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/752/2/94

Publication URI: http://dx.doi.org/10.1088/0004-637x/752/2/94

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2

ISSN: 0004-637X