A thin-shell model shows that radio-emitting outflows from tidal disruption events expand with a t^(2/3) law under black hole gravity, allowing SMBH masses to be estimated from observed shell radius and velocity.
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Mass Determination of Supermassive Black Holes Governing Evolution of Radio Emitters
A thin-shell model shows that radio-emitting outflows from tidal disruption events expand with a t^(2/3) law under black hole gravity, allowing SMBH masses to be estimated from observed shell radius and velocity.