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Cited article:
G. Lanzafame , G. Belvedere , D. Molteni
A&A, 453 3 (2006) 1027-1036
Published online: 2006-06-28
This article has been cited by the following article(s):
8 articles
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Implicit integrations for SPH in semi-Lagrangian approach: Application to the accretion disc modeling in a microquasar
G. Lanzafame Computer Physics Communications 184 (3) 671 (2013) https://doi.org/10.1016/j.cpc.2012.11.001
Measuring the effects of artificial viscosity in SPH simulations of rotating fluid flows
P. A. Taylor and J. C. Miller Monthly Notices of the Royal Astronomical Society 426 (2) 1687 (2012) https://doi.org/10.1111/j.1365-2966.2012.21747.x
An approach to solving the boundary free edge difficulties in SPH modelling: application to a viscous accretion disc in close binaries
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Modelling shear flows with smoothed particle hydrodynamics and grid-based methods
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Effects of local thermodynamics and of stellar mass ratio on accretion disc stability in close binaries
G. Lanzafame Astronomische Nachrichten 330 (8) 843 (2009) https://doi.org/10.1002/asna.200811243
Artificial viscosity in simulation of shock waves by smoothed particle hydrodynamics
M. Nejad-Asghar, A. R. Khesali and J. Soltani Astrophysics and Space Science 313 (4) 425 (2008) https://doi.org/10.1007/s10509-007-9712-4
Role of Compressibility, Turbulent Viscosity, and Mass-Transfer-Rate on Accretion Discs in Close Binaries
Giuseppe Lanzafame Publications of the Astronomical Society of Japan 60 (2) 259 (2008) https://doi.org/10.1093/pasj/60.2.259