Theoretical framework for precessing TDE disks predicts variable IR dust echo light curves showing double-to-single peaked profile transitions due to viewing and precession angle changes.
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Larger black holes in TDEs accrete more material and launch faster winds, with unbound mildly relativistic winds for higher viscosity parameters and bound convective outflows for lower ones.
3D hydro simulations show that TDE outflow interactions with a broken power-law CNM can reproduce the range of observed radio light curves via early flares inside the Bondi radius and possible late rebrightenings outside it.
citing papers explorer
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Infrared Echoes of Precessing Tidal Disruption Events
Theoretical framework for precessing TDE disks predicts variable IR dust echo light curves showing double-to-single peaked profile transitions due to viewing and precession angle changes.
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Hydrodynamical simulation of wind production from hot accretion flows in tidal disruption events
Larger black holes in TDEs accrete more material and launch faster winds, with unbound mildly relativistic winds for higher viscosity parameters and bound convective outflows for lower ones.
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Simulations of interaction between outflow and surrounding broken power-law circumnuclear medium: implications for different radio light curves of TDEs
3D hydro simulations show that TDE outflow interactions with a broken power-law CNM can reproduce the range of observed radio light curves via early flares inside the Bondi radius and possible late rebrightenings outside it.
- Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks