The past and future evolution of a star like Betelgeuse

@article{Meynet2013ThePA,
  title={The past and future evolution of a star like Betelgeuse},
  author={G. Meynet and L. Haemmerl{\'e} and S. Ekstrom and C. Georgy and J. Groh and A. Maeder},
  journal={Eas Publications Series},
  year={2013},
  volume={60},
  pages={17-28}
}
We discuss the physics and the evolution of a typical massive star passing through an evolutionary stage similar to that of Betelgeuse. After a brief introduction recalling various observed parameters of Betelgeuse, we discuss the Pre-Main-Sequence phase (PMS), the Main-Sequence (MS) phase, the physics governing the duration of the first crossing of the HR diagram, the red supergiant stage (RSG), the post-red supergiant phases and the final fate of solar metallicity stars with masses between 9… Expand
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