Numerical Models of Accretion Disks
arXiv:astro-ph/9712233 · doi:10.1063/1.55861
Abstract
I review recent numerical studies of accretion disks, focusing on measurements of the turbulent shear stress, or , in the shearing box model. I conclude with a list of astronomically relevant open questions that can be settled via future numerical experiments.
9 pages, LaTeX, aipproc.sty, invited review at "Accretion Processes in Astrophysical Systems: Some Like It Hot", eds. S. Holt and T. Kallman