Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-25T14:34:40.715Z Has data issue: false hasContentIssue false

Optically Quiet Quasars

Published online by Cambridge University Press:  04 August 2017

W. D. Cotton*
Affiliation:
National Radio Astronomy Observatory

Extract

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.

The study of steep spectrum sources containing compact components has become increasingly popular as the number of papers on the topic in this volume indicates. I wish to discuss the properties of a number of steep spectrum sources which are dominated by compact components whose spectra remain steep to quite low frequencies. Most of the known sources of this type do not have optical counterparts to the limit of the Palomar Sky Survey prints and thus, with the implicit assumption that they are extragalactic, have been referred to as “Optically Quiet Quasars”.

Type
Research Article
Copyright
Copyright © Reidel 1984 

References

Condon, J. J. and Ledden, J. E.: 1981, Astron. J. 86, pp. 643652.CrossRefGoogle Scholar
Cotton, W. D.: 1976, Astrophys. J. 204, pp. L63L66.CrossRefGoogle Scholar
Cotton, W. D.: 1983, Astrophys. J. in press.Google Scholar
Cotton, W. D., Owen, F. N., Geldzahler, B. J., Johnston, K., Baath, L. B. and Romney, J.: 1983, submitted to Astrophys. J. Google Scholar
Gower, J.F.R., Scott, P. F. and Wills, D.: 1967, Mem. Roy. Astron. Soc. 71, pp. 49144.Google Scholar
Owen, F. N., Condon, J. J. and Ledden, J. E.: 1983, Astron. J. 88, pp. 115.CrossRefGoogle Scholar
Sharp, J. R. and Bash, F. N.: 1975, Astron. J. 80, pp. 335352.Google Scholar
Spangler, S. R. and Cotton, W. D.: 1981, Astron. J. 86, pp 730746.Google Scholar
Terrell, J.: 1966, Science 154, pp. 1281.Google Scholar