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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3 Pith papers cite this work, alongside 6 external citations. Polarity classification is still indexing.
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Anomalous pre-intersection dissipation in TDE simulations is numerical in origin, arising from pericenter kinematics combined with algorithm sensitivities to converging versus diverging flows.
Presents a four-module LLM framework for text-to-SQL on the ALeRCE astro database, evaluated on 110 NL/SQL pairs across 13 models with perfect-match metrics.
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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On the origin of anomalous dissipation in simulations of tidal disruption events
Anomalous pre-intersection dissipation in TDE simulations is numerical in origin, arising from pericenter kinematics combined with algorithm sensitivities to converging versus diverging flows.
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Querying an astronomical database using large language models: the ALeRCE text-to-SQL system
Presents a four-module LLM framework for text-to-SQL on the ALeRCE astro database, evaluated on 110 NL/SQL pairs across 13 models with perfect-match metrics.