Hostname: page-component-5c6d5d7d68-txr5j Total loading time: 0 Render date: 2024-08-15T20:11:53.786Z Has data issue: false hasContentIssue false
  • English
  • Français

A dependence between optical and radio luminosities of quasars after all?

Published online by Cambridge University Press:  19 July 2016

Jerzy Machalski
Jerzy Machalski*
Affiliation:
Astronomical Observatory, Jagellonian University, ul. Orla 171, PL-30244 Cracow, Poland

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.

It is still uncertain whether optical and radio emission mechanisms in AGNs are coupled or not, and how? New observational data give more light on this subject.

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 109 - 110
Copyright
Copyright © Reidel 1986 

References

Bahcall, J.N., and Turner, E.L. (1977). IAU Symp. No. 74, p. 295 Google Scholar
Fanti, R., and Perola, G.C.(1977). IAU Symp. No. 74, 171 Google Scholar
Machalski, J., and Condon, J.J.(1985). A.J. (submitted) Google Scholar
Macklin, J.T. (1982). M.H.R.A.S. 199, 1119 Google Scholar