Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-26T13:31:23.335Z Has data issue: false hasContentIssue false

Quasar Contribution to the X-Ray Background

Published online by Cambridge University Press:  14 August 2015

Ajit Kembhavi
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, England
A. C. Fabian
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, England

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.

Recent observations by the Einstein Observatory have shown that a majority of known quasars are powerful X-ray emitters. The 107 objects observed as of Feb. 1980 (Zamorani et al. 1980) have X-ray, optical and radio luminosities scattered over a wide range. Until a large enough X-ray selected sample of quasars becomes available, it is necessary to study statistical correlations in the available sample, so that some insight into X-ray production may be obtained, and the contribution of quasars to the X-ray background estimated.

Type
Research Article
Copyright
Copyright © Reidel 1981 

References

Braccesi, A., Zitelli, V., Bonoli, F., and Formiggini, L.: 1980, Astron. Astrophys., 85, pp 8092.Google Scholar
Cavaliere, A., Danese, L., De Zotti, G., and Franceschini, A.: 1980, Preprint.Google Scholar
Fabian, A.C., and Rees, M.J.: 1978, MNRAS, 185, pp 109122.Google Scholar
Smith, M.C., and Wright, A.E.: 1979, Anglo-Australian Observatory, Preprint.Google Scholar
Zamorani, G. et al.: 1980, Preprint.Google Scholar