Abstract
OBSERVATIONS of the early September 1972 flare of the radio counterpart of Cyg X-3 were made at 3.3 mm (90 GHz) with the 4.6-m antenna of the Aerospace Corporation. Observing and data reduction procedures identical to those described by Fogarty et al.1 yielded the 3.3 mm total fluxes (E-W linear polarization) given in Table 1.
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References
Fogarty, W. G., Epstein, E. E., Montgomery, J. W., and Dworetsky, M. M., Astron. J., 76, 537 (1971).
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POMPHREY, R., EPSTEIN, E. Cygnus X-3: 3.3 mm Observations. Nature Physical Science 239, 125–126 (1972). https://doi.org/10.1038/physci239125b0
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DOI: https://doi.org/10.1038/physci239125b0
