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Volumn 289, Issue 4, 1997, Pages 889-897
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Reproducing superhumps and γ-shifts of SU UMa stars with SPH simulations
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Author keywords
Accretion, accretion discs; Hydrodynamics; Novae, cataclysmic variables
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Indexed keywords
MASS TRANSFER;
STARS;
THERMODYNAMIC STABILITY;
VISCOSITY;
ACCRETION DISCS;
ACCRETION: ACCRETION DISKS;
HYDRODYNAMIC SIMULATION;
LIGHT CURVES;
MASS RATIO;
NOVAE CATACLYSMIC VARIABLES;
ORBITALS;
SMOOTHED PARTICLE HYDRODYNAMICS;
TEMPORAL DEVELOPMENT;
TWO-DIMENSIONAL;
HYDRODYNAMICS;
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EID: 0000659169
PISSN: 00358711
EISSN: None
Source Type: Journal
DOI: 10.1093/mnras/289.4.889 Document Type: Article |
Times cited : (16)
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References (18)
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