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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 

References

Fanti, C., Fanti, R., Ficarra, A., Gregorini, L., Mantovani, F., Padrielli, L. 1983, Astron.Astrophys. 118, 171 Google Scholar
Hunstead, R.W. 1972, Astrophys.Lett. 12, 193 Google Scholar
McAdam, W.B. 1976, Proc.astr.Soc.Aust. 3, 86 Google Scholar
McAdam, W.B. 1978, Proc.astr.Soc.Aust. 3, 283 CrossRefGoogle Scholar
McAdam, W.B. 1980, Proc.astr.Soc.Aust. 4, 70 Google Scholar