The resonant B1II+B1II binary BI108

Details The resonant B1II+B1II binary BI108 The resonant B1II+B1II binary BI108

2010-09-17

arxiv.org/abs/1009.3511v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

2 pages, 1 figure, IAUS 272 - Active OB Stars: Structure, Evolution, Mass Loss and Critical Limits

Scientific paper

BI108 is a luminous variable star in the Large Magellanic Cloud classified
B1II. The variability consists of two resonant periods (3:2), of which only one
is orbital, however. We discuss possible mechanisms responsible for the second
period and its resonant locking.

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