The Circumstellar Environments of the Cool Hypergiants: Implications for the Mass Loss Mechanism
The cool hypergiants are the most luminous known stars in the upper HR Diagram in the apparent temperaturerange represented by the spectral types A to M. Most of these stars in this regime are unstable as evidenced bytheir high mass loss rates, variability, and in some cases large IR excesses and ci...
Zapisane w:
| Wydane w: | Revista Mexicana de Astronomía y Astrofísica |
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| 1. autor: | |
| Format: | Artigo |
| Język: | Inglês |
| Wydane: |
Universidad Nacional Autónoma de México
2007
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| Hasła przedmiotowe: | |
| Dostęp online: | https://www.redalyc.org/articulo.oa?id=57130003 |
| Etykiety: |
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