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Published online by Cambridge University Press: 20 January 2011
Tidal disruption by massive black holes is a phenomenon, during which a large part ofgravitational energy can be released on a very short time-scale. The time-scales andenergies involved during X-ray and IR flares observed in Galactic centre suggest that theymay be related to tidal disruption events. Furthermore, aftermath of a tidal disruption ofa star by super-massive black hole has been observed in some galaxies, e.g.RX J1242.6-1119A. All these discoveries increased the demand for tools for tidaldisruption study in curved space-time. Here we summarise our study of general relativisticeffects on tidal deformation of stars and compact objects.