Abstract
A CONTINUING programme to measure the visibility of radio sources and monitor the possible variability in their angular structure is in progress by collaboration between the Algonquin Radio Observatory, Lake Traverse, Ontario (operated by the National Research Council of Canada) and the Field Station at Chilbolton, England (operated by the Radio and Space Research Station of the UK Science Research Council). As an initial result the visibility curve for 3C84, taken in November 1972, is presented here, with two possible interpretations.
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References
Broten, N. W., Clarke, R. W., Legg, T. H., Locke, J. L., Galt, J. A., Yen, J. L., and Chisholm, R. M., Mon. Not. R. astr. Soc., 146, 313 (1969).
Kellermann, K. I., and Pauliny-Toth, I. I. K., Astrophys. J. Lett., 155, L71 (1969).
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LEGG, T., BROTEN, N., FORT, D. et al. Long Baseline Interferometry of the Seyfert Galaxy 3C84. Nature 244, 18–19 (1973). https://doi.org/10.1038/244018a0
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DOI: https://doi.org/10.1038/244018a0
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