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arXiv · 1204.4561

The signature of tidal disruption phenomena in the vicinity of a black hole

Uros Kostic·Andrej Cadez·Massimo Calvani·Claudio Germana
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Abstract

Tidal effects on clumps of material during random non-stationary accretion onto a black hole produce phenomena with distinct temporal characteristics in observed light-curves. During such non-stationary accretion events, the shape of the accreting object evolves in time, and observable quasi-periodic phenomena with variable quasi-periods are produced. A number of characteristic light-curves, obtained with numerical simulations, will be shown. Their relevance to observed phenomena will be briefly discussed.

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Uros Kostic, Andrej Cadez, Massimo Calvani, Claudio Germana. 2012-04-20. The signature of tidal disruption phenomena in the vicinity of a black hole. https://doi.org/10.1142/9789814374552_0096

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