UBV LIGHT CURVES OF V356 SAGITTARII

We report here UBV observations of the unusual eclipsing binary V356 S agittarii from 1973, 1974, and 1975. Although there are phase gaps, li ght-curve form and absolute level differ only slightly from light curv es of 23 years earlier in the phases that are covered. Scatter is anom alously large, as in the earlier observations, and seems to be diagnos tic of some intrinsic abnormality.