Stellar-mass black holes dragging gas from accretion disks out to their Hill radius can power quasi-periodic eruptions, while stellar impactors produce too-asymmetric and tidally unstable flares.
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Quasi-periodic Eruptions from Stellar-mass Black Holes Impacting Accretion Disks in Galactic Nuclei
Stellar-mass black holes dragging gas from accretion disks out to their Hill radius can power quasi-periodic eruptions, while stellar impactors produce too-asymmetric and tidally unstable flares.