A time-dependent model shows that star-disk collisions in TDE systems hosting EMRIs can eject 10^{-3} to 1 solar masses at 0.02-0.1c years after the initial flare, producing radio emission via interaction with circumnuclear material.
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4 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 4years
2026 4representative citing papers
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.
Faint radio emission in TDE2025aarm implies a collimated outflow from unbound debris with solid angle ≲0.1 sr, while X-rays can arise from the same shock via synchrotron or inverse-Compton scattering.
citing papers explorer
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Delayed Radio Flares in Tidal Disruption Events from Star-Disk Collision Outflows
A time-dependent model shows that star-disk collisions in TDE systems hosting EMRIs can eject 10^{-3} to 1 solar masses at 0.02-0.1c years after the initial flare, producing radio emission via interaction with circumnuclear material.
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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.
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On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm
Faint radio emission in TDE2025aarm implies a collimated outflow from unbound debris with solid angle ≲0.1 sr, while X-rays can arise from the same shock via synchrotron or inverse-Compton scattering.