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VLBI observations of galactic nuclei at 18 centimeters - NGC 1052, NGC 4278, M82, and M104Compact radio sources about a light year in size have been detected in the nuclei of the galaxies NGC 1052, NGC 3034 (M82), NGC 4278, and NGC 4594 (M104) at a wavelength of 18 cm. The compact nucleus detected in M81 at 6 cm was not seen at 18 cm. The compact source in M82 is unique among extragalactic sources in its size-spectrum relationship. It is either broadened by scattering within M82 or it lies behind, and is absorbed by, an H II region. In these galaxies, the size of the nuclear radio source at 18 cm is larger than it is at higher frequencies. The nucleus of the giant radio galaxy DA 240 was not detected.
Document ID
19800029913
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Shaffer, D. B.
(National Radio Astronomy Observatory Green Bank, W. Va., United States)
Marscher, A. P.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 10, 2013
Publication Date
November 1, 1979
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
80A14083
Funding Number(s)
CONTRACT_GRANT: NSF AST-77-00247
CONTRACT_GRANT: NSF AST-77-00440
Distribution Limits
Public
Copyright
Other

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