• Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of α Eri and β CMi 

      Rubio, A. C.; Carciofi, A. C.; Ticiani, P.; Mota, B. C.; Vieira, R. G.; Faes, D. M.; Genaro, M.; Amorim, T. H. de; Klement, R.; Araya, I. [Centro de Óptica e Información Cuántica, Vicerrectoría de Investigación, Universidad Mayor, Chile]; Arcos, C.; Cure, M.; Souza, A. Domiciano de; Georgy, C.; Jones, C. E.; Suffak, M. W.; Silva, A. C. F. (Oxford University Press, 2023-09)
      Classical B emission (Be) stars are fast rotating, near-main-sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars. Our goal is to infer stellar ...


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