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High-Resolution Observations of Variable Radio Sources
Published online by Cambridge University Press: 14 August 2015
Abstract
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Preliminary results are reported of a long-term program to test models of variable radio sources by direct observations of diameter changes. Although further confirmation is needed, increase in angular diameter attributed to a centimetric component of 3C 279 found in 1966 implies relativistic expansion with α ≳ 2.
In order to sort out events taking place in variable sources it is necessary to observe frequently and at many wavelengths, especially at short wavelengths.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 44: External Galaxies and Quasi-Stellar Objects , 1972 , pp. 228 - 229
- Copyright
- Copyright © Reidel 1972
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