Classical Be stars

@article{Rivinius2013ClassicalBS,
  title={Classical Be stars},
  author={Th. Rivinius and Alex C. Carciofi and Christophe Martayan},
  journal={The Astronomy and Astrophysics Review},
  year={2013},
  volume={21},
  pages={1-86}
}
In the past decade, a consensus has emerged regarding the nature of classical Be stars: They are very rapidly rotating main sequence B stars, which, through a still unknown, but increasingly constrained process, form an outwardly diffusing gaseous, dust-free Keplerian disk. In this work, first the definition of Be stars is contrasted to similar classes, and common observables obtained for Be stars are introduced and the respective formation mechanisms explained. We then review the current state… Expand
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