Evolution of self-gravitating magnetized disks. II. Interaction between magnetohydrodynamic turbulence and gravitational instabilities

We present three-dimensional magnetohydrodynamic (MHD) numerical simulations of the evolution of self-gravitating and weakly magnetized disks with an adiabatic equation of state. Such disks are subject to the development of both the magnetorotational and gravitational instabilities, which transport...

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Detalles Bibliográficos
Autores principales: Fromang, S, Balbus, S, Terquem, C, De Villiers, J
Formato: Journal article
Lenguaje:English
Publicado: Institute of Physics Publishing 2004

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