Abstract
Braes and Miley1, using the Westerbork synthesis array operating at 1,415 MHz, have detected a variable radio source associated with the X-ray source Cyg X-3. This letter reports observations of the radio counterpart of Cyg X-3 at 2,695 and 8,085 MHz with the NRAO interferometer at spacings of 2,400, 1,900 and 500 m.
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References
Braes, L. L. E., and Miley, G. K., Nature, 237, 506 (1972).
Giacconi, R., Murray, S., Gursky, H., Kellogg, E., Schreier, E., and Tananbaum, H., Astrophys. J. (in the press).
Hjellming, R. M., and Wade, C. M., Astrophys. J., 164, L1 (1971).
Wade, C. M., and Hjellming, R. M., Astrophys. J., 170, 532 (1971).
Wade, C. M., and Hjellming, R. M., Nature, 235, 270 (1972).
Hjellming, R. M., Wade, C. M., and Webster, E., Nature, 236, 43 (1972).
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HJELLMING, R., HERMANN, M. & WEBSTER, E. Radio Observations of Cygnus X-3. Nature 237, 507–508 (1972). https://doi.org/10.1038/237507a0
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DOI: https://doi.org/10.1038/237507a0
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