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Home All issues A&A, 399 2 (2003) 395-407 Article references

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Cited article:

FARGOCPT: 2D Multiphysics code for simulating disk interactions with stars, planets, and particles

Thomas Rometsch, Lucas M. Jordan, Tobias W. Moldenhauer, Dennis Wehner, Steven Rendon Restrepo, Tobias W. A. Müller, Giovanni Picogna, Wilhelm Kley and Cornelis P. Dullemond
Astronomy & Astrophysics 684 A192 (2024)
https://doi.org/10.1051/0004-6361/202348687

Measuring the numerical viscosity in simulations of protoplanetary disks in Cartesian grids

Jibin Joseph, Alexandros Ziampras, Lucas Jordan, George A. Turpin and Richard P. Nelson
Astronomy & Astrophysics 678 A134 (2023)
https://doi.org/10.1051/0004-6361/202245601

Estimates of the evolution of small perturbations in the radial spread (drain) of a viscous ring

D. V. Georgievskii and G. S. Tlyustangelov
Journal of Applied Mechanics and Technical Physics 58 (4) 610 (2017)
https://doi.org/10.1134/S0021894417040046

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

Interaction between massive planets on inclined orbits and circumstellar discs

M. Xiang-Gruess and J. C. B. Papaloizou
Monthly Notices of the Royal Astronomical Society 431 (2) 1320 (2013)
https://doi.org/10.1093/mnras/stt254

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

How initial and boundary conditions affect protoplanetary migration in a turbulent sub-Keplerian accretion disc: 2D non-viscous SPH simulations

V. Costa, V. Pirronello, G. Belvedere, et al.
Monthly Notices of the Royal Astronomical Society 401 (4) 2388 (2010)
https://doi.org/10.1111/j.1365-2966.2009.15815.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

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

NUMERICAL DISSIPATION IN RSPH SIMULATIONS OF ASTROPHYSICAL FLOWS WITH APPLICATION TO PROTOPLANETARY DISKS

S. Børve, R. Speith and J. Trulsen
The Astrophysical Journal 701 (2) 1269 (2009)
https://doi.org/10.1088/0004-637X/701/2/1269

Spectral Methods for Time‐dependent Studies of Accretion Flows. I. Two‐dimensional, Viscous, Hydrodynamic Disks

Chi‐kwan Chan, Dimitrios Psaltis and Feryal Ozel
The Astrophysical Journal 628 (1) 353 (2005)
https://doi.org/10.1086/430511

Simulations of planet-disc interactions using Smoothed Particle Hydrodynamics

C. Schäfer, R. Speith, M. Hipp and W. Kley
Astronomy & Astrophysics 418 (1) 325 (2004)
https://doi.org/10.1051/0004-6361:20034034