SPH simulations of spiral shocks in discs around black holes

Publications of the Astronomical Society of Japan

Volumn 54, Issue 5, 2002, Pages 781-785

  Belvedere, Gaetano ^a   Lanzafame, Giuseppe ^b  

^a UNIVERSITY OF CATANIA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

Author keywords

Accretion, accretion disks; Methods: numerical; Shock waves; Stars: binary: close; Stars: cataclysmic variables

Indexed keywords

BLACK HOLES; COMPRESSIBILITY; GAS DYNAMICS; GRAVITATION; HYDRODYNAMICS; NUMERICAL METHODS; STARS;

2-D MODEL; ACCRETION: ACCRETION DISKS; CATACLYSMIC VARIABLES; METHOD: NUMERICAL; SHOCK-WAVES; SMOOTH PARTICLE HYDRODYNAMICS; SPIRAL STRUCTURES; STAR: CATACLYSMIC VARIABLE; STARS:BINARIES CLOSE; STARS:CATACLYSMIC;

SHOCK WAVES;

EID: 0036457563     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/54.5.781     Document Type: Article

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