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Benjamin Amend

1 articles · 5 co-authors · latest: 2026-06-01

Fading Black Hole Flares: The Key Is the Star's Rapid Spin

Some repeating partial tidal disruption events show flares that fade from one to the next—a phenomenon that contradicted old models. Hydrodynamic simulations reveal that the culprit is the rapid initial prograde spin of a star captured via the Hills mechanism: the tidal torque is inefficient, and ma
arXiv:2606.02692v1 · 2026-06-01