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Cited article:

GLOBAL MHD SIMULATIONS OF ACCRETION DISKS IN CATACLYSMIC VARIABLES. I. THE IMPORTANCE OF SPIRAL SHOCKS

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The Astrophysical Journal 823 (2) 81 (2016)
https://doi.org/10.3847/0004-637X/823/2/81

GodunovSPH with shear viscosity: implementation and tests

Seung-Hoon Cha and Matt A. Wood
Monthly Notices of the Royal Astronomical Society 458 (1) 480 (2016)
https://doi.org/10.1093/mnras/stw402

Collective molecular dissipation on Navier–Stokes macroscopic scales: Accretion disc viscous modeling in SPH

Giuseppe Lanzafame
International Journal of Modern Physics D 24 (03) 1550028 (2015)
https://doi.org/10.1142/S0218271815500285

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)
https://doi.org/10.1111/j.1365-2966.2010.17218.x

An approach to the Riemann problem in the light of a reformulation of the state equation for SPH inviscid ideal flows: a highlight on spiral hydrodynamics in accretion discs

G. Lanzafame
Monthly Notices of the Royal Astronomical Society 408 (4) 2336 (2010)
https://doi.org/10.1111/j.1365-2966.2010.17283.x

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

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

Low compressibility accretion disc formation in close binaries: the role of physical viscosity

G. Lanzafame, G. Belvedere and D. Molteni
Astronomy & Astrophysics 453 (3) 1027 (2006)
https://doi.org/10.1051/0004-6361:20054225