Mhd waves in stellar winds and accretion disks
Alfven waves have been used to explain the heating of stellar coronae andthe production of stellar winds in many regions of the Hertzsprung-Russell (HR)diagram. The waves were used as a major acceleration mechanism in the wind ofprotostars, late-type stars, early-type stars and in the solar wind. Th...
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
2000
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| Θέματα: | |
| Διαθέσιμο Online: | https://www.redalyc.org/articulo.oa?id=57100918 |
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