Pearson, T. J. and Readhead, A. C. S. (1984) VLBI Survey of a Complete Sample of Active Nuclei and Quasars. In: VLBI and Compact Radio Sources. IAU Symposium Proceedings Series. No.110. D. Reidel , Dordrecht, pp. 15-24. ISBN 9789027717399. https://resolver.caltech.edu/CaltechAUTHORS:20181211-081238775
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Abstract
We have conducted a VLBI survey of a complete, flux-density limited sample of 65 extragalactic radio sources, selected at 5 GHz. We have made hybrid maps at 5 GHz of all of the sources accessible to the Mark-II system. The sources can be divided provisionally into a number of classes with different properties: central components of extended double sources, steep-spectrum compact sources, very compact (almost unresolved) sources, asymmetric sources (sometimes called “core-jet” sources), and “compact double” sources. It is not yet clear whether any of these classes is physically distinct from the others, or whether there is a continuous range of properties.
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| Additional Information: | © 1984 by the IAU. VLBI research at the Owens Valley Radio Observatory is supported by NSF grant AST 82-10259. We are very grateful to the U.S. Network, the Max-Planck Institut für Radioastronomie, and the staffs of the observatories, for making the observations possible. | ||||||
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| Series Name: | IAU Symposium Proceedings Series | ||||||
| Issue or Number: | 110 | ||||||
| Record Number: | CaltechAUTHORS:20181211-081238775 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20181211-081238775 | ||||||
| Official Citation: | Pearson, T., & Readhead, A. (1984). VLBI Survey of a Complete Sample of Active Nuclei and Quasars. Symposium - International Astronomical Union, 110, 15-24. doi:10.1017/S007418090007755X | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 91667 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Tony Diaz | ||||||
| Deposited On: | 11 Dec 2018 18:12 | ||||||
| Last Modified: | 03 Oct 2019 20:37 |
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