The Magneto-Rotational Instability in Protoplanetary Disks

We review the current understanding of how mass accretion takes place in protoplanetary disks. Particular emphasis is placed on the role played by the magneto-rotational instability (MRI) in the transport of angular momentum across the disk. We discuss the conditions for the development of the MRI i...

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Udgivet i:Revista Mexicana de Astronomía y Astrofísica
Main Authors: F. J. Sánchez Salcedo, E. Pérez Tijerina, Mauricio Reyes Ruiz
Format: Artigo
Sprog:Inglês
Udgivet: Universidad Nacional Autónoma de México 2003
Fag:
Física, Astronomía y Matemáticas
Hydrodynamics
Unstabilities
Accretion : Accretion Disks
Planetary Systems : Formation
Online adgang:https://www.redalyc.org/articulo.oa?id=57101824
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