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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):
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The slow decline of the Galactic recurrent novae T Pyxidis, IM Normae, and CI Aquilae
Andrea Caleo and Steven N. Shore
Monthly Notices of the Royal Astronomical Society 449 (1) 25 (2015)
DOI: 10.1093/mnras/stv265
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Implicit integrations for SPH in semi-Lagrangian approach: Application to the accretion disc modeling in a microquasar
G. Lanzafame
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DOI: 10.1016/j.cpc.2012.11.001
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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)
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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)
DOI: 10.1093/pasj/60.2.259
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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)
DOI: 10.1007/s10509-007-9712-4
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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)
DOI: 10.1002/asna.200811243
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An approach to solving the boundary free edge difficulties in SPH modelling: application to a viscous accretion disc in close binaries
G. Lanzafame
Monthly Notices of the Royal Astronomical Society 408 (3) 1551 (2010)
DOI: 10.1111/j.1365-2966.2010.17218.x
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