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The LMC star BI 108 is photometrically variable with the unique light curve:Two strong periods are present in a strict 3:2 resonance, staying coherent overseveral observing seasons. A spectroscopic data collected at VLT/UVES revealsunexpected and still not fully understood behavior of the system, that has notbeen observed in any other early-type multiple systems.

The study of resonant variability observed in the massive LMC system BI 108