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Fe K features as probes of the nuclear reflection region in Seyfert galaxiesThe warm electron scattering region posited in 1985 by Antonucci and Miller to exist in NGC 1068 may be a characteristic feature of Seyfert galaxies. Whenever it exists, it presents a unique signature in Fe X-ray features. Predictions of the strength of the Fe K-edge and K-alpha line in both type 1 and type 2 Seyfert galaxies are presented and interpreted.
Document ID
19880023114
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/184966
Authors
Krolik, Julian H. (Johns Hopkins University Baltimore, MD; California, University, Santa Barbara, United States)
Kallman, Timothy R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1987
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 320
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
88A10341
Funding Number(s)
CONTRACT_GRANT: NSF PHY-82-17853
CONTRACT_GRANT: NAGW-1017
Distribution Limits
Public
Copyright
Other

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