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IRAS observations of radio-quiet and radio-loud quasarsObservations from 12 to 100 microns are presented of two radio-quiet and three radio-loud quasars. Over this wavelength range, all five have grossly similar continuum energy distributions. The continua of the radio-loud quasars are consistent with synchrotron radiation. There is an indication, however, of excess 100 micron emission in the two radio-quiet quasars.
Document ID
19840044932
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Neugebauer, G.
(California Inst. of Tech. Pasadena, CA, United States)
Soifer, B. T.
(California Institute of Technology Pasadena, CA, United States)
Miley, G.
(California Inst. of Tech. Pasadena, CA, United States)
Habing, H. J.
(Leiden, Rijksuniversiteit, Sterrewacht Leiden, Netherlands)
Young, E.
(California Inst. of Tech. Pasadena, CA, United States)
Low, F. J.
(Steward Observatory Tucson, AZ, United States)
Beichman, C. A.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Clegg, P. E.
(California Inst. of Tech. Pasadena, CA, United States)
Harris, S.
(California Inst. of Tech. Pasadena, CA, United States)
Rowan-Robinson, M.
(Queen Mary College London, United Kingdom)
Date Acquired
August 12, 2013
Publication Date
March 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 278
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
84A27719
Distribution Limits
Public
Copyright
Other

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