Abstract
Photometric observations of primary minimum inU, B, andV filters have been discussed. The amplitude of variation in all the three filters is 0m.66. We do not find variations in the period and its revised value is 1d.0047115.
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Srivastava, J.B., Kandpal, C.D. Eclipsing binary UW Bootis. Astrophys Space Sci 133, 291–296 (1987). https://doi.org/10.1007/BF00642488
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DOI: https://doi.org/10.1007/BF00642488