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Dynamics of accretion and winds in tidal disruption events

By T. Mageshwaran and Arun Mangalam at
LogoTata Institute of Fundamental Research
and
LogoIndian Institute of Astrophysics
We have constructed self-similar models of a time-dependent accretion disk in both sub and super-Eddington phases with wind outflows for tidal disruption events (TDEs). The physical input parameters are the black hole (BH) mass \(M_{\bullet}\), specific orbital energy \(E\) and angular momentum \(J\), star mass \(M_{\star}\) and radius \(R_{\star}\). We... Show more
August 14, 2020
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Dynamics of accretion and winds in tidal disruption events
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