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Superluminal motion in compact radio sourcesThe observations of radio sources whose components appear to move superluminally are now sufficient to eliminate certain theoretical models. However, a number of models might be still relevant. The models which involve relativistic bulk motions of the radio components seem to provide the most likely explanation of apparent superluminal motion. A summary of observational predictions of various models for superluminal motions is included.
Document ID
19800051525
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Marscher, A. P.
(California, University San Diego, Calif., United States)
Scott, J. S.
(Steward Observatory Tucson, Ariz., United States)
Date Acquired
August 10, 2013
Publication Date
May 1, 1980
Publication Information
Publication: Astronomical Society of the Pacific
Subject Category
Astrophysics
Accession Number
80A35695
Distribution Limits
Public
Copyright
Other

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