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A disk around one component of a binary star system with sufficiently highinclination can undergo Kozai-Lidov (KL) oscillations during which the diskinclination and disk eccentricity are exchanged. Previous studies show thatwithout a source of accretion, KL unstable disks exhibit damped oscillations,due to viscous dissipation, that leave the disk stable near or below thecritical inclination for KL oscillations. With three-dimensional hydrodynamicalsimulations we show that a highly misaligned circumbinary disk that flows ontothe binary components forms highly inclined circumstellar disks around eachcomponent. We show that a continuous infall of highly inclined material allowsthe KL oscillations to continue. The KL disk oscillations produce shocks andeccentricity growth in the circumstellar disks that affect the conditions forplanet formation.

Sustained Kozai-Lidov oscillations in misaligned circumstellar gas disks