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Elliptical Accretion Disk as a Model for Tidal Disruption Events

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Tidal Disruptions of Main-sequence Stars. I. Observable Quantities and Their Dependence on Stellar and Black Hole Mass

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The post-maximum behaviour of the changing-look Seyfert galaxy NGC 1566

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Tidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations

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NTT,SPITZER, ANDCHANDRASPECTROSCOPY OF SDSSJ095209.56+214313.3: THE MOST LUMINOUS CORONAL-LINE SUPERNOVA EVER OBSERVED, OR A STELLAR TIDAL DISRUPTION EVENT?

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Tidal Disruption of Stellar Objects by Hard Supermassive Black Hole Binaries

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