Stellar parameters and H α line profile variability of Be stars in the BeSOS survey

@article{Arcos2018StellarPA,
  title={Stellar parameters and H $\alpha$ line profile variability of Be stars in the BeSOS survey},
  author={C Arcos and Samer Kanaan and Joseph P'aez Ch'avez and Leonardo Vanzi and Ignacio J Araya and Michel Cur'e},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018},
  volume={474},
  pages={5287-5299}
}
The Be phenomenon is present in about 20$\%$ of the B-type stars. Be stars show variability on a broad range of timescales, which in most cases is related to the presence of a circumstellar disk of variable size and structure. For this reason a time resolved survey is highly desirable in order to understand the mechanisms of disk formation which are still poorly understood. In addition, a complete observational sample would improve the statistical significance of the study of the stellar and… 
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