Finite, intense accretion bursts from tidal disruption of stars on bound orbits

We study accretion processes for tidally disrupted stars approaching supermassive black holes on bound orbits, by performing three-dimensional smoothed particle hydrodynamics simulations with a pseudo-Newtonian potential. We find that there is a critical value of the orbital eccentricity below which...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2013-09, Vol.434 (2), p.909-924
Hauptverfasser: Hayasaki, Kimitake, Stone, Nicholas, Loeb, Abraham
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Sprache:eng
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