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• W1866782783 startingPage "75" @default.
• W1866782783 abstract "Martin et al. showed that a substantially misaligned accretion disk around one component of a binary system can undergo global damped Kozai–Lidov (KL) oscillations. During these oscillations, the inclination and eccentricity of the disk are periodically exchanged. However, the robustness of this mechanism and its dependence on the system parameters were unexplored. In this paper, we use three-dimensional hydrodynamical simulations to analyze how various binary and disk parameters affect the KL mechanism in hydrodynamical disks. The simulations include the effect of gas pressure and viscosity, but ignore the effects of disk self-gravity. We describe results for different numerical resolutions, binary mass ratios and orbital eccentricities, initial disk sizes, initial disk surface density profiles, disk sound speeds, and disk viscosities. We show that the KL mechanism can operate for a wide range of binary-disk parameters. We discuss the applications of our results to astrophysical disks in various accreting systems." @default.
• W1866782783 created "2016-06-24" @default.
• W1866782783 creator A5014975239 @default.
• W1866782783 creator A5051918386 @default.
• W1866782783 creator A5080080275 @default.
• W1866782783 date "2015-07-01" @default.
• W1866782783 modified "2023-09-25" @default.
• W1866782783 title "THE KOZAI–LIDOV MECHANISM IN HYDRODYNAMICAL DISKS. II. EFFECTS OF BINARY AND DISK PARAMETERS" @default.
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• W1866782783 doi "https://doi.org/10.1088/0004-637x/807/1/75" @default.
• W1866782783 hasPublicationYear "2015" @default.
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