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Dynamic Spectra of Low-Frequency Variables

Published online by Cambridge University Press:  04 August 2017

Brian Dennison
Affiliation:
Physics Dept., Virginia Polytechnic Institute and State University
J. J. Broderick
Affiliation:
Physics Dept., Virginia Polytechnic Institute and State University
S. L. O'Dell
Affiliation:
Physics Dept., Virginia Polytechnic Institute and State University
K. J. Mitchell
Affiliation:
Physics Dept., Virginia Polytechnic Institute and State University
D. R. Altschuler
Affiliation:
Physics Dept., University of Puerto Rico
H. E. Payne
Affiliation:
National Radio Astronomy Observatory
J. J. Condon
Affiliation:
National Radio Astronomy Observatory

Extract

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A wide range of models have been proposed to account for low-frequency (≲ 1 GHz) variability in cosmologically-distant radio sources. To address these models we (Payne et al. 1982) are monitoring the 0.3–1.4 GHz spectra of such sources. Results from three years of monitoring indicate that two distinct types of low-frequency variables may exist.

Type
Research Article
Copyright
Copyright © Reidel 1984 

References

Aller, H. D., and Aller, M. F.: 1982, in Green Bank Workshop on Low-Frequency Variability, eds. Cotton, W. D. and Spangler, S. R., 105.Google Scholar
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Fanti, C., Fanti, R., Ficarra, A., Gregorini, L., Montovani, F., and Padrielli, L.: 1983, Astron. Astrophys. 118, 171.Google Scholar
Payne, H. E. Altschuler, D. R., Broderick, J. J., Condon, J. J., Dennison, B., and O'Dell, S. L.: 1982, in Green Bank Workshop on Low-Frequency Variability, eds. Cotton, W. D. and Spangler, S. R., 9.Google Scholar