The Evolution of Circumstellar Medium around Rotating Massive Stars
A rotating 12 M star, after its main-sequence evolution, becomes a redsupergiant when it starts core Heburning. During core helium burning, as consequence of a variation of the hydrogen shell burning eciency,the star undergoes a so called \blue loop", i.e. it evolves into a blue supergiant stage, wh...
Αποθηκεύτηκε σε:
| Εκδόθηκε σε: | Revista Mexicana de Astronomía y Astrofísica |
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| Κύριοι συγγραφείς: | , , , |
| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
Universidad Nacional Autónoma de México
2007
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| Θέματα: | |
| Διαθέσιμο Online: | https://www.redalyc.org/articulo.oa?id=57130014 |
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