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Far-infrared variability in active galactic nucleiPointed IRAS observations of 20 active galaxies were examined in the first detailed search for far-infrared variability in a large sample of active galaxies. Less extensive survey data were also checked for evidence of strong 6-month variability in 45 active galaxies. The far-infrared fluxes of three highly polarized objects ('blazars') appeared to vary by up to a factor of 2 on time scales of a few months. No convincing cases of variability greater than about 15 percent (rms) were found in any of the normal quasars or Seyfert galaxies studied. It appears that blazars tend to be variable at all wavelengths, but most active galaxies may be systematically less variable in the far-infrared than at higher frequencies.
Document ID
19880036357
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Edelson, R. A.
(Owens Valley Radio Observatory, Pasadena, CA; Colorado, University Boulder, United States)
Malkan, M. A.
(California, University Los Angeles, United States)
Date Acquired
August 13, 2013
Publication Date
December 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 323
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
88A23584
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-52643
CONTRACT_GRANT: NSF AST-83-14134
CONTRACT_GRANT: NAS7-918
Distribution Limits
Public
Copyright
Other

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