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The resonant B1II+B1II binary BI108

Solar and Stellar Astrophysics 2015-05-20 v1
Authors: Th. Rivinius , R. E. Mennickent , Z. Kołaczkowski
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Abstract

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.

Cite

@article{arxiv.1009.3511,
  title  = {The resonant B1II+B1II binary BI108},
  author = {Th. Rivinius and R. E. Mennickent and Z. Kołaczkowski},
  journal= {arXiv preprint arXiv:1009.3511},
  year   = {2015}
}

Comments

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

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