Tidal disruption of a star by a supermassive blackhole

Details Tidal disruption of a star by a supermassive blackhole Tidal disruption of a star by a supermassive blackhole

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254...48l&link_type=abstract

Testing the AGN paradigm diagnostics. AIP Conference Proceedings, Volume 254, pp. 48-51 (1992).

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Black Holes, Hydrodynamics, Relativity And Gravitation

Scientific paper

The analysis of stars in galactic nuclei that are captured and tidally disrupted by a black hole of mass <106Msolar requires the inclusion of general relativistic effects. We present the first numerical study of tidal breakup of a 1Msolar main sequence star by a 107Msolar black hole. We use a smoothed particle code to solve the hydrodynamic equations for a relativistic fluid in a static curved spacetime geometry to analyze, among other things, the fraction of the debris captured by the hole and the velocity of fragments escaping the hole.

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