Spiral structures and shocks in accretion discs in close binary systems: The role of the stellar mass ratio

Publications of the Astronomical Society of Japan

Volumn 52, Issue 3, 2000, Pages 515-522

  Lanzafame, Giuseppe ^a   Maravigna, Fabio ^b   Belvedere, Gaetano ^b  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b UNIVERSITY OF CATANIA   (Italy)

Author keywords

Accretion, accretion discs; Binaries: close; Hydrodynamics; Methods: numerical; Shock fronts

Indexed keywords

HYDRODYNAMICS; NUMERICAL METHODS; RADIAL FLOW; STARS; SYSTEMS (METALLURGICAL);

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BINARY SYSTEMS; MASS RATIO; METHOD: NUMERICAL; SHOCK FRONTS; SMOOTH PARTICLE HYDRODYNAMICS; SPIRAL STRUCTURES; STELLAR MASS;

SHOCK WAVES;

EID: 0034341960     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/52.3.515     Document Type: Article

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