Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-29T22:55:48.189Z Has data issue: false hasContentIssue false
  • English
  • Français

Correlation Between Extended Radio and Line Emission for a Radio-loud Quasar Sample

Published online by Cambridge University Press:  13 May 2016

Xinwu Cao  and
D.R. Jiang
Xinwu Cao
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, National Astronomical Observatories, China
D.R. Jiang
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, National Astronomical Observatories, China

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.

A strong correlation is present between the extended radio and broad-line emission for a radio-loud quasar sample. The statistic behaviour on the core emission of lobe-dominated quasars is rather different from that of core-dominated quasars. The extended radio luminosity is a good tracer for jet power, while the core luminosity can only be a jet power tracer for core-dominated quasars.

Type
The Inner Regions of Galaxies
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 150 - 151
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Cao, X., Jiang, D.R., 1999, MNRAS 307, 802.CrossRefGoogle Scholar
Falcke, H., Biermann, P., 1995, A&A 293, 665.Google Scholar
Rawlings, S. G., Saunders, R. D. E., 1991, Nat 349, 138.CrossRefGoogle Scholar
Xu, C., Livio, M., 1999, AJ 118, 1169.CrossRefGoogle Scholar