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Characterization of X-ray sources detected in a deep Einstein exposure of the field around 3C 295An extensive set of optical and radio observations is presented that characterize the X-ray sources detected in an extremely deep Einstein Observatory exposure of the 3C 295 region. A total of five X-ray sources was found. This number is consistent with the only previous log N - log S result published at these flux levels. One of the sources was a galactic star. The four extragalactic sources are active galactic nuclei (three Seyferts and one QSO). Two of the sources are Seyfert galaxies in the 3C 295 cluster, one of which was previously unknown. The number of Seyfert galaxies in the cluster that is found from this complete X-ray survey is inconsistent with that expected from the fraction of low-redshift active galactic nuclei in their clusters.
Document ID
19850060929
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Henry, J. P.
(Hawaii Univ. Honolulu, HI, United States)
Lavery, R. J.
(Hawaii, University Honolulu, United States)
Clarke, J. T.
(Hawaii Univ. Honolulu, HI, United States)
Bowyer, S.
(California, University Berkeley, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: Astronomical Journal
Volume: 90
ISSN: 0004-6256
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-6256
Accession Number
85A43080
Funding Number(s)
CONTRACT_GRANT: NAG8-458
CONTRACT_GRANT: NSF AST-80-05874
Distribution Limits
Public
Copyright
Other

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