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Tidal disruption of stars by a massive black hole
Authors:Oded Regev  Daniel Portnoy
Institution:(1) Department of Physics, Technion-Israel Institute of Technology, Haifa, Israel
Abstract:The hydrodynamics of stellar models in the tidal field of a massive black hole is calculated numerically under certain simplifying assumptions. It is found that solar type stars are totally disrupted only when falling toward a black hole whose mass does not exceed 106–107 M odot. Red giants lose their entire envelope for all black hole masses studied.Our findings strengthen the view that tidal disruption is not an important source of gas in AGN's.
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