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The VLBI core in Radio Loud AGNs

Published online by Cambridge University Press:  13 May 2016

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

Abstract

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We present statistical results on VLBI cores from large VLBI samples at C, L and S/X bands. Most of the results are consistent with the inhomogeneous jet model. The magnetic field distribution and particle density in the inhomogeneous jet model were estimated. We also found that the flux densities and luminosities of the cores at 5 GHz were correlated with those at optical band in the rest-frame.

Type
The Inner Regions of Galaxies
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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