Abstract
Two groups have reported analyses of photometric1,2 and spectroscopic3 data of Sco X-1, which suggest a binary nature. Prior to these studies no persistent periodic variations of the X-ray flux have been found, but the first group1 claims a periodic variation in the light curve of 3.93 d with a mean amplitude of 0.8 mag, and the second2 claims variations of 0.22 mag in amplitude, with a period of 0.787 d.
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DE FREITAS PACHECO, J. Origin of the optical emission from Sco X-1. Nature 253, 699–701 (1975). https://doi.org/10.1038/253699a0
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DOI: https://doi.org/10.1038/253699a0
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