Large-amplitude modulations and hours-timescale variability in the early X-ray light curve of a tidal disruption flare

We present new X-ray, optical, and UV observations of the tidal disruption event candidate eRASSt J234402.9−352640 (hereafter J2344). Between 50 and 60 days after peak optical brightness, J2344 exhibited large-amplitude modulations in its 0.2−2 keV emission, when the flux repeatedly dimed and re-brightened by a factor of ∼6 over a ∼3-day timescale. These modulations exhibited harder-when-brighter behaviour but were not detected in high-cadence observations obtained 60−70 days and 170−200 days after peak optical brightness, when the system instead exhibited stochastic X-ray variability over timescales of hours. We discuss the different physical mechanisms responsible for such exotic X-ray variability and explore the possibility that the modulations in J2344 were caused by the Lense-Thirring precession of the inner accretion flow around the disrupting black hole.