Substantial stream-disc overflow found in three-dimensional SPH simulations of cataclysmic variables

Monthly Notices of the Royal Astronomical Society

Volumn 322, Issue 3, 2001, Pages 499-514

  Kunze, Stefan ^a   Speith, Roland ^a   Hessman, Frederic V ^b  

^a UNIVERSITY OF TÜBINGEN   (Germany)

^b UNIVERSITY OF GÖTTINGEN   (Germany)

Author keywords

Accretion, accretion discs; Binaries: general; Hydrodynamics; Novae, cataclysmic variables; Stars: dwarf novae

Indexed keywords

ASTROPHYSICS; MASS TRANSFER; X RAY ABSORPTION;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BINARIES:GENERAL; CATACLYSMIC VARIABLES; DISK SURFACES; DWARF NOVAE; MASS TRANSFER RATE; NOVAE CATACLYSMIC VARIABLES; ORBITAL PHASE; STARS: DWARF NOVAE;

HYDRODYNAMICS;

EID: 0001542922     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04057.x     Document Type: Article

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