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Modelling the light-curves of objects tidally disrupted by a black hole

Published online by Cambridge University Press:  20 January 2011

H. Wozniak ,
G. Hensler ,
U. Kostić ,
A. Gomboc ,
A. Čadež  and
M. Calvani
U. Kostić
Affiliation:
Department of Physics, Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000 Ljubljana, Slovenia
A. Gomboc
Affiliation:
Department of Physics, Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000 Ljubljana, Slovenia
A. Čadež
Affiliation:
Department of Physics, Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000 Ljubljana, Slovenia
M. Calvani
Affiliation:
INAF, Astronomical Observatory of Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy
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Abstract

Tidal disruption by massive black holes is a phenomenon, during which a large part of gravitational energy can be released on a very short time-scale. The time-scales and energies involved during X-ray and IR flares observed in Galactic centre suggest that they may be related to tidal disruption events. Furthermore, aftermath of a tidal disruption of a 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 tidal disruption study in curved space-time. Here we summarise our study of general relativistic effects on tidal deformation of stars and compact objects.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 44: JENAM 2008: Grand Challenges in Computational Astrophysics , 2010 , pp. 125 - 126
Copyright
© EAS, EDP Sciences 2011

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References

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