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...
Wedi'i Gadw mewn:
| Cyhoeddwyd yn: | Revista Mexicana de Astronomía y Astrofísica |
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| Prif Awduron: | , , , |
| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
Universidad Nacional Autónoma de México
2009
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| Pynciau: | |
| Mynediad Ar-lein: | https://www.redalyc.org/articulo.oa?id=57115743022 |
| Tagiau: |
Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!
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