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The very flat radio spectrum of 0735 plus 178 - A cosmic conspiracyMultifrequency interferometric and total flux density measurements of the radiation from 0735 plus 178 are discussed. It is shown that it is far more likely that the very flat radio spectrum of this source results from a superposition of incoherent synchrotron radiation from four distinct, homogeneous components, each with a peaked spectrum, than from radiation from a single inhomogeneous component.
Document ID
19800061053
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/183271
Authors
Cotton, W. D. (Massachusetts Inst. of Tech. Cambridge, MA, United States)
Wittels, J. J. (Massachusetts Inst. of Tech. Cambridge, MA, United States)
Shapiro, I. I. (Massachusetts Inst. of Tech. Cambridge, MA, United States)
Marcaide, J. (MIT Cambridge, Mass., United States)
Owen, F. N. (Massachusetts Inst. of Tech. Cambridge, MA, United States)
Spangler, S. R. (National Radio Astronomy Observatory Charlottesville, Va., United States)
Rius, A. (Instituto Nacional de Tecnica Aerospacial Madrid, Spain)
Angulo, C. (Escuela Tecnica Superior de Ingenieros de Telecomunicacion Barcelona, Spain)
Clark, T. A. (NASA Goddard Space Flight Center Greenbelt, Md., United States)
Knight, C. A. (Haystack Observatory Westford, Mass., United States)
Date Acquired
August 10, 2013
Publication Date
June 15, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
80A45223
Funding Number(s)
CONTRACT_GRANT: NGR-22-009-839
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NSF GP-25865
CONTRACT_GRANT: NSF EAR-76-22615
Distribution Limits
Public
Copyright
Other

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