Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.
2021b, MNRAS
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astro-ph.HE 2years
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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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.