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

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

2010-04-30

arxiv.org/abs/1004.5464v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

2 pages, 1 figure. To appear in ASP Conference Series special issue: "Binaries: Key to Comprehension of the Universe".

Scientific paper

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 over
several observing seasons. A spectroscopic data collected at VLT/UVES reveals
unexpected and still not fully understood behavior of the system, that has not
been observed in any other early-type multiple systems.

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