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

We present 3D 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 angular moment...

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Bibliográfalaš dieđut
Váldodahkkit: Fromang, S, Balbus, S, Terquem, C, Villiers, J
Materiálatiipa: Journal article
Almmustuhtton: 2004