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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 gravitati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27c8115d3f7acf965297557f25daa150
https://ora.ox.ac.uk/objects/uuid:4c68433e-d471-4b56-ae64-a1e6a48a95c8
https://ora.ox.ac.uk/objects/uuid:4c68433e-d471-4b56-ae64-a1e6a48a95c8
