Kozai-Lidov oscillations of a tilted Be-star disc can reproduce the roughly three-year recurrence of giant X-ray outbursts in 4U 0115+634, provided the disc is not fully destroyed and retains eccentric material.
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The frequency of Kozai-Lidov disc oscillation driven giant outbursts in Be/X-ray binaries
Kozai-Lidov oscillations of a tilted Be-star disc can reproduce the roughly three-year recurrence of giant X-ray outbursts in 4U 0115+634, provided the disc is not fully destroyed and retains eccentric material.