Radio Observations of an Ordinary Outflow from the Tidal Disruption Event AT2019dsg
Open Access
- 1 October 2021
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 919 (2), 127
- https://doi.org/10.3847/1538-4357/ac110a
Abstract
We present detailed radio observations of the tidal disruption event (TDE) AT2019dsg, obtained with the Karl G. Jansky Very Large Array (VLA) and the Atacama Large Millimeter/submillimeter Array (ALMA), and spanning 55-560 days post disruption. We find that the peak brightness of the radio emission increases until similar to 200 days and subsequently begins to decrease steadily. Using a standard equipartition analysis, including the effects of synchrotron cooling as determined by the joint VLA-ALMA spectral energy distributions, we find that the outflow powering the radio emission is in roughly free expansion with a velocity of approximate to 0.07 c, while its kinetic energy increases by a factor of about 5 from 55 to 200 days and plateaus at approximate to 4.4 x 10(48) erg thereafter. The ambient density traced by the outflow declines as radius approximate to R (-1.7) on a scale of approximate to(1-4) x 10(16) cm (approximate to 6300-25,000 R ( s )), followed by a steeper decline to approximate to 7 x 10(16) cm (approximate to 44,000 R ( s )). Allowing for a collimated geometry, we find that to reach even mildly relativistic velocities (Gamma = 2) the outflow requires an opening angle of theta ( j ) approximate to 2 degrees, which is narrow even by the standards of gamma-ray burst jets; a truly relativistic outflow requires an unphysically narrow jet. The outflow velocity and kinetic energy in AT2019dsg are typical of previous non-relativistic TDEs, and comparable to those from type Ib/c supernovae, raising doubts about the claimed association with a high-energy neutrino event.Funding Information
- Space Telescope Science Institute (HST-HF2-51403.001-A)
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