Hostname: page-component-848d4c4894-sjtt6 Total loading time: 0 Render date: 2024-06-24T05:23:54.354Z Has data issue: false hasContentIssue false
  • English
  • Français

Relativistic Beaming and Quasar Statistics

Published online by Cambridge University Press:  14 August 2015

I.W.A. Browne  and
M.J.L. Orr
I.W.A. Browne
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire
M.J.L. Orr
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire

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.

The predictions of a scheme which attributes the observed differences between flat and steep spectrum quasars to projection and the effects of relativistic beaming are explored. We conclude that the statistical properties of quasars are entirely consistent with such a scheme provided the mean Lorentz factor in the central components of quasars is ∼5.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 169 - 172
Copyright
Copyright © Reidel 1982 

References

Condon, J.J. and Ledden, J.E., (1981). preprint.Google Scholar
Orr, M.J.L. and Browne, I.W.A., (1981). In preparation.Google Scholar
Scheuer, P.A.G. and Readhead, A.C.S. (1979). Nature 277, 182.Google Scholar