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GCVS Team
32 Cyg. Probably enters a common system with V695 Cyg (31 Cyg). 0 < d < 0.011P. P var. Min I = 2420670.0 + 1140.1d*E (JD2411400 - 29700). Since JD2429700 - see Table. The epoch of the eclipse of the B4 type Component by the K5 type component is given. There is also small physical light variability of the K component [G.Hill, G.L.C.Aikman, R.W.Hilditch, E.L.Pfannenschmidt, P.F.Younger, Victoria Publ 15, N10, 389, 1980., E.Guinan, G.McCook, M.Garhart, BAAS 14, 543, 1982.]. Depth of eclipses depends of lambda: 0.04M V, 0.13m B, 0.27m (lambda 4243A),0.90m (lambda 3552A).
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