作者: Wen Fu , Stephen H. Lubow , Rebecca G. Martin
DOI: 10.1088/0004-637X/807/1/75
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摘要: Martin et al. (2014b) showed that a substantially misaligned accretion disk around one component of binary system can undergo global damped Kozai-Lidov oscillations. During these oscillations, the inclination and eccentricity are periodically exchanged. However, robustness this mechanism its dependence on parameters were unexplored. In paper, we use three-dimensional hydrodynamical simulations to analyze how various affect in disks. The include effect gas pressure viscosity, but ignore effects self-gravity. We describe results for different numerical resolutions, mass ratios orbital eccentricities, initial sizes, surface density profiles, sound speeds, viscosities. show operate wide range binary-disk parameters. discuss applications our astrophysical disks accreting systems.