Three-dimensional numerical simulation of gaseous flow structure in semidetached binaries

Monthly Notices of the Royal Astronomical Society

Volumn 300, Issue 1, 1998, Pages 39-48

  Bisikalo, D V ^a   Boyarchuk, A A ^a   Chechetkin, V M ^b   Kuznetsov, O A ^b   Molteni, D ^c  

^a INSTITUTE OF ASTRONOMY   (Russian Federation)

^b KELDYSH INSTITUTE OF APPLIED MATHEMATICS   (Russian Federation)

^c UNIVERSITY OF PALERMO   (Italy)

Author keywords

Accretion, accretion discs; Binaries: close; Hydrodynamics; Methods: numerical; Stars: mass loss

Indexed keywords

GAS DYNAMICS; GASES; MASS TRANSFER; MORPHOLOGY; NUMERICAL METHODS; NUMERICAL MODELS; SHOCK WAVES; STARS;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; HOTSPOTS; MASS TRANSFER RATE; METHOD: NUMERICAL; NONMAGNETICS; SHOCK-WAVES; STARS: MASS-LOSS; THREE-DIMENSIONAL NUMERICAL SIMULATIONS;

FLOW STRUCTURE;

EID: 0002618375     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01815.x     Document Type: Article

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