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...

Descrición completa

Gardado en:
Detalles Bibliográficos
Publicado en:Revista Mexicana de Astronomía y Astrofísica
Main Authors: F. J. Sánchez Salcedo, E. Pérez Tijerina, Mauricio Reyes Ruiz
Formato: Artigo
Idioma:Inglês
Publicado: Universidad Nacional Autónoma de México 2003
Assuntos:
Física, Astronomía y Matemáticas
Hydrodynamics
Unstabilities
Accretion : Accretion Disks
Planetary Systems : Formation
Acceso en liña:https://www.redalyc.org/articulo.oa?id=57101824
Tags: Engadir etiqueta
Sen Etiquetas, Sexa o primeiro en etiquetar este rexistro!

Títulos similares