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Hydrodynamic modelling of accretion flows

J. R. Murray·M. R. Truss·S. B. Foulkes·C. A. Haswell·K. Manson
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Abstract

In the proceedings of this, and of several recent close binary conferences, there have been several contributions describing smoothed particle hydrodynamics simulations of accretion disks. It is apposite therefore to review the numerical scheme itself with emphasis on its advantages for disk modelling, and the methods used for modelling viscous processes.

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J. R. Murray, M. R. Truss, S. B. Foulkes, C. A. Haswell, K. Manson. 2004-03-18. Hydrodynamic modelling of accretion flows. https://arxiv.org/abs/astro-ph/0403434

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