Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-08T05:37:35.570Z Has data issue: false hasContentIssue false

VLBI Survey of a Complete Sample of Active Nuclei and Quasars

Published online by Cambridge University Press:  04 August 2017

T. J. Pearson
Affiliation:
Owens Valley Radio Observatory, California Institute of Technology
A.C.S. Readhead
Affiliation:
Owens Valley Radio Observatory, California Institute of Technology

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Research Article
Copyright
Copyright © Reidel 1984 

References

Browne, I.W.A., Clark, R.R., Moore, P.K., Muxlow, T.W.B., Wilkinson, P.N., Cohen, M.H., and Porcas, R.W.: 1982, Nature 299, pp. 788793.CrossRefGoogle Scholar
Cornwell, T.J., and Wilkinson, P.N.: 1981, Monthly Notices Roy. Astron. Soc. 196, pp. 10671086.CrossRefGoogle Scholar
Kühr, H., Pauliny-Toth, I.I.K., Witzel, A., and Schmidt, J.: 1981a, Astron. J. 86, pp. 854863.CrossRefGoogle Scholar
Kühr, H., Witzel, A., Pauliny-Toth, I.I.K., and Nauber, U.: 1981b, Astron. Astrophys. Suppl. 45, pp. 367430.Google Scholar
Linfield, R.: 1981, Astrophys. J. 244, pp. 436446.CrossRefGoogle Scholar
Owen, F.N., Spangler, S.R., and Cotton, W.D.: 1980, Astron. J. 85, pp. 351362.CrossRefGoogle Scholar
Pauliny-Toth, I.I.K., Witzel, A., Preuss, E., Kühr, H., Kellermann, K.I., Fomalont, E.B., and Davis, M.M.: 1978, Astron J. 83, pp. 451474.CrossRefGoogle Scholar
Pearson, T.J., and Readhead, A.C.S.: 1981, Astrophys. J. 248, pp. 6181.CrossRefGoogle Scholar
Perley, R.A.: 1982, Astron. J. 87, pp. 859880.CrossRefGoogle Scholar
Phillips, R.B., and Mutel, R.L.: 1982, Astron. Astrophys. 106, pp. 2124.Google Scholar
Porcas, R.W.: 1981, Nature, 294, pp. 4749.CrossRefGoogle Scholar
Preuss, E., Kellermann, K.I., Pauliny-Toth, I.I.K., and Shaffer, D.B.: 1980, Astrophys. J. 240, pp. L7L10.CrossRefGoogle Scholar
Readhead, A.C.S., Pearson, T.J., and Unwin, S.C.: 1984, IAU Symp. No.110 this volume p. 131.CrossRefGoogle Scholar
Rudnick, L., and Jones, T.W.: 1982, Astrophys. J. 255, pp. 3947.CrossRefGoogle Scholar
Rudnick, L., and Jones, T.W.: 1983, Astron. J. 88, pp. 518526.CrossRefGoogle Scholar
Seielstad, G.A., Pearson, T.J., and Readhead, A.C.S.: 1983, Publ. Astron. Soc. Pacific, in press.Google Scholar
Simon, R.S.: 1982, , California Institute of Technology.Google Scholar