We performed CCD photometric observations of W UMa type contact binary BV Dra during eight nights from May 1996 to June 1999 using 61cm telescope at Sobaeksan Optical Astronomy Observatory. and completed BVR light curves of the system. From our observations. we derived nine new times of minimum lights (five timings for primary eclipse. https://mabelandfoxs.shop/product-category/tights/
Tights
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