机译:Low compressibility accretion disc formation in close binaries: the role of physical viscosity
INAF, Osservatorio Astrofis Catania, I-95123 Catania, Italy;
Catania Univ, Sez Astrofis, Dipartimento Fis & Astron, I-95123 Catania, Italy;
Univ Palermo, Dipartimento Fis & Tecnol Relat, I-90128 Palermo, Italy;
accretion; accretion discs; stars : binaries : close; stars : dwarf novae; white dwarfs; methods : numerical; methods : N-body simulations; SMOOTHED PARTICLE HYDRODYNAMICS; SPIRAL SHOCKS; DWARF NOVAE; 3D SIMULATIONS; MASS-TRANSFER; COSMOLOGICAL SIMULATIONS; NUMERICAL SIMULATIONS; SPH SIMULATIONS; WIND ACCRETION; BLACK-HOLES;