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• W2000767881 abstract "Abstract This paper describes a code that has been written to simulate viscous accretion flows that possess angular momentum. An explicit Eulerian flux-corrected-transport (FCT) algorithm is used to perform advection of the fluid, which is a perfect gas. An alternating-directions-implicit (ADI) scheme is used to calculate viscous diffusion. The viscous dissipation of energy can be included if desired. The code has been used to model the viscous boundary layer between a thin Keplerian accretion disc and a non-rotating star, and the viscous evolution of a thick accretion torus. Further details are described by Robertson and Frank." @default.
• W2000767881 created "2016-06-24" @default.
• W2000767881 creator A5032089806 @default.
• W2000767881 date "1987-06-01" @default.
• W2000767881 modified "2023-10-14" @default.
• W2000767881 title "Axisymmetric accretion flows in astrophysics" @default.
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• W2000767881 doi "https://doi.org/10.1016/0010-4655(87)90083-x" @default.
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