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MG12 - Talk detail
 

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 Participant 

Kostic, Uros

Institution

Uiversity of Ljubljana  - Jadranska 19 - Ljubljana - - Slovenia

Session

Talk

Abstract

APT1

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

Tidal effects on clumps of material during random nonstationary accretion onto a black hole produce phenomena with distinct temporal characteristics in observed light-curves. During such nonstationary accretion the shape evolves in time, which produces observable quasi-periodic phenomena with variable quasiperiods. A number of characteristic light-curves, obtained with numerical simulations will be shown, and their relevance to observed phenomena will be briefly discussed.

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