MAGNETIZED DISKS AROUND YOUNG STARS
We discuss the structure and evolution of a magnetized accretion disks around young stars that have dragged their magnetic eld in the process of gravitational collapse. The disk evolves due to two di usive processes: viscous stresses that redistribute mass and angular momentum, and the resistive di...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2009
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57115743022 |
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