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IRAS observations of NGC 1052The galaxy NGC 1052 has been observed with the IRAS satellite. The infrared emission at 100 microns is substantially larger than a smooth extrapolation of the radio data. Because of the large diaphragm size of IRAS, it is impossible to decide uniquely if the infrared radiation represents a self-absorbed nonthermal spectrum or thermal reradiation by heated dust.
Document ID
19850039910
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)
Rice, W.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Rowan-Robinson, M.
(Queen Mary College London, United Kingdom)
Date Acquired
August 12, 2013
Publication Date
December 1, 1984
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 96
ISSN: 0004-6280
Subject Category
Astrophysics
Accession Number
85A22061
Distribution Limits
Public
Copyright
Other

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