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Monitoring of Southern QSOs at 843 MHz

Published online by Cambridge University Press:  07 August 2017

W.B. McAdam
W.B. McAdam*
Affiliation:
School of Physics, University of Sydney, N.S.W. 2006, Australia

Abstract

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A sample of more than 100 southern QSOs is being monitored for flux density variations by the Molonglo Observatory Synthesis Telescope (MOST). Provisional results for an interval of 4 years shows that the variability at 843 MHz is less than at 408 MHz. There seems to be a real ‘mid-frequency gap’ with little variability near 1 GHz.

Type
Part 10: Radio Galaxies, Components and Structure
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 539 - 540
Copyright
Copyright © Kluwer 1989 

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