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 opposite therefore to review the numerical scheme itself with emphasis on its advantages for disk modelling, and the methods used for modelling viscous processes.
Original language | English |
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Pages (from-to) | 166-168 |
Number of pages | 3 |
Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volume | 20 |
Publication status | Published - 2004 |
Event | IAU Colloquium 194 - Compact Binaries in the Galaxy and Beyond - La Paz, B.C. Sur, Mexico Duration: 17 Nov 2003 → 22 Nov 2003 |