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

Astronomy and Astrophysics

Volumn 453, Issue 3, 2006, Pages 1027-1036

  Lanzafame, G ^a   Belvedere, G ^b   Molteni, D ^c  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b UNIVERSITY OF CATANIA   (Italy)

^c UNIVERSITY OF PALERMO   (Italy)

Author keywords

Accretion, accretion discs; Methods: N body simulations; Methods: numerical; Stars: binaries: close; Stars: dwarf novae, white dwarfs

Indexed keywords

ASTROPHYSICS; COMPRESSIBILITY; COMPUTER SIMULATION; GAS DYNAMICS; GRAVITATION; HYDRODYNAMICS; NUMERICAL METHODS; VISCOSITY; WAVE PROPAGATION;

ACCRETION, ACCRETION DISCS; BINARY SYSTEM; METHODS: N-BODY SIMULATIONS; SMOOTH PARTICLE HYDRODYNAMICS (SPH); STARS: BINARIES: CLOSE; STARS: DWARF NOVAE, WHITE DWARFS;

GALAXIES;

EID: 33746044167     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054225     Document Type: Article

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