What powers the radio emission in TDE AT2019dsg: a long-lived jet or the disruption itself?
Tatsuya Matsumoto, Tsvi Piran, and Julian H. Krolik

TL;DR
The radio emission in TDE AT2019dsg can be explained by a single plasma ejection rather than ongoing energy injection from a central engine, with the event resembling an early supernova remnant stage.
Contribution
This study demonstrates that continuous energy injection is unnecessary to explain the radio data, proposing a single ejection model supported by equipartition analysis.
Findings
Radio energy increases as t^{0.7}
The emitting region expands at ~0.06c
Energy is supplied by the outflow, not ongoing injection
Abstract
The tidal disruption event AT2019dsg was observed from radio to X-rays and was possibly accompanied by a high-energy neutrino. Previous interpretations have focused on continued injection by a central engine as the source of energy for radio emission. We show that continuous energy injection is unnecessary; the radio data can be explained by a single ejection of plasma that supplies all the energy needed. To support this assertion, we analyze the synchrotron self-absorbed spectra in terms of the equipartition model. Similar to previous analyses, we find that the energy in the radio-emitting region increases approximately and the lengthscale of this region grows at a rate . This event resembles the earliest stage of a supernova remnant: because the ejected mass is much greater than the shocked external mass, its velocity remains unchanged, while…
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