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

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,...

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Published inarXiv.org
Main Authors Kołaczkowski, Zbigniew, Mennickent, Ronald, Rivinius, Thomas
Format Paper
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 30.04.2010
Subjects
Light curve
Photometry
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Abstract 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.
AbstractList 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.
Author Kołaczkowski, Zbigniew
Rivinius, Thomas
Mennickent, Ronald
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Title The study of resonant variability observed in the massive LMC system BI 108
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