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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

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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