Supersonic wind accretion in massive close binary systems: A 3D SPH simulation of Cen X-3

Monthly Notices of the Royal Astronomical Society

Volumn 295, Issue 3, 1998, Pages 618-622

  Lanzafame, G ^a   Belvedere, G ^b  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b UNIVERSITY OF CATANIA   (Italy)

Author keywords

Accretion, accretion discs; Binaries: close; Hydrodynamics; Methods: numerical; Stars: individual: Cen X 3

Indexed keywords

NUMERICAL METHODS; SYSTEMS (METALLURGICAL); WHITE DWARFS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BINARY SYSTEMS; INDIVIDUAL:CEN X-3; METHOD: NUMERICAL; SPH SIMULATION; STAR: INDIVIDUAL: CEN X-3; STARS: INDIVIDUAL: PROXIMA CENTAURI; STRUCTURE AND DYNAMICS; SUPERSONIC WIND ACCRETION;

HYDRODYNAMICS;

EID: 0001652342     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01374.x     Document Type: Article

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