Abstract
We discuss photometric monitoring (VBLUW system) of three B(e) supergiants. All three objects appear to be variable. They are subject to two (R 66 and R 126 in the LMC) and three (S 18 in the SMC) types of light oscillations which range from a few days to years, and are probably due to pulsations. We argue that a classication as Cyg variables is justied. Their classication as mixed B(e)/S Dor variables is less certain, though not impossible. Also based on other cases, a strong B(e){S Dor variable connection seems to be present.
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