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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2026 2representative citing papers
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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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.