Hydrodynamic modelling of accretion flows
Astrophysics
2007-05-23 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/0403434,
title = {Hydrodynamic modelling of accretion flows},
author = {J. R. Murray and M. R. Truss and S. B. Foulkes and C. A. Haswell and K. Manson},
journal= {arXiv preprint arXiv:astro-ph/0403434},
year = {2007}
}
Comments
3 pages, to appear in proceedings of IAU Colloquium 194: Compact binaries in the galaxy and beyond