Abstract
A 4.8 hour periodicity in the X-ray intensity of Cygnus X-3 has been reported1–3. The Uhuru observations of May 8 to May 17, 1972, show a smooth, nearly sinusoidal modulation of about half the source intensity1–2. The Copernicus data3, which have a similar appearance, were collected during September 1972. This was after the first outburst of a radio source4,5 which may be associated with Cygnus X-3. We present here a study of the time variability of the X-ray intensity of Cygnus X-3 with data collected by the OSO-7 satellite in December 1971 and in January, June and July 1972.
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References
Brinkman, A., Parsignault, D., Giacconi, R., Gursky, H., Kellogg, E., Schreier, E., and Tananbaum, H., IAU Circ, No. 2446 (1972).
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Clark, G. W., Bradt, H. V., Lewin, W. H. G., Markert, T. H., Schnopper, H. W., and Sprott, G. F., Astrophys. J. (in the press).
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CANIZARES, C., McCLINTOCK, J., CLARK, G. et al. Observations of Periodic Variations in the X-ray Intensity of Cygnus X-3. Nature Physical Science 241, 28–30 (1973). https://doi.org/10.1038/physci241028a0
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DOI: https://doi.org/10.1038/physci241028a0
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