Be star demographics: a comprehensive study of thousands of lightcurves in the Magellanic Clouds
A. L. Figueiredo, A. C. Carciofi, J. Labadie-Bartz, M. L. Pinho, T. H. de Amorin, P. T. dos Santos, I. Soszy\'nski, A. Udalski

TL;DR
This comprehensive study analyzes 20-year light curves of around 3000 Be stars in the Magellanic Clouds, revealing differences in activity and disk behavior related to metallicity.
Contribution
It provides the first detailed comparison of Be star variability and disk properties across two different metallicity environments using extensive long-term data.
Findings
Higher duty cycle in SMC compared to LMC.
Disks are almost always present in these stars.
Lower metallicity stars show more activity and longer outbursts.
Abstract
Multi-color OGLE survey light curves of about 20 years duration are analyzed for about 3000 classical Be stars in the Large and Small Magellanic Clouds (LMC, SMC) in order to study the properties and variability. Each light curve was manually analyzed to distinguish between different scenarios, such as photospheric baseline levels, and disk build-up and dissipation phases. This analysis was aided by dynamical disk models and photospheric models to coarsely determine inclination angle and mass. Measured quantities such as the fraction of time spent actively ejecting mass (the duty cycle), the fraction of time spent with a detectable disk (the disk duty cycle), the build-up and dissipation time of isolated disk events, and the number of mass outbursts per year allow us to characterize and compare the behavior of the two populations. There is a wide spread in the duty cycle, with median…
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