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...
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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autor: | |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2007
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57130003 |
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