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The highly obscured nucleus of 3C 219The detection of a strong, and possibly broad, Paschen-alpha line from the narrow-line radio galaxy 3C 219 is reported. The detected flux is larger than predicted from the H-alpha line and the case B recombination. This implies the presence of a highly reddened line-emitting region in the nucleus.
Document ID
19860055118
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/184666
Authors
Fabbiano, G. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Willner, S. P. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Carleton, N. P (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Elvis, M. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
May 15, 1986
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 304
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
86A39856
Funding Number(s)
CONTRACT_GRANT: NAS8-30751
Distribution Limits
Public
Copyright
Other

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