Starfall: A heavy rain of stars in 'turning on' AGN
B.McKernan, K.E.S. Ford, M. Cantiello, M.J. Graham, A.S. Jermyn,, N.W.C. Leigh, T. Ryu, D. Stern

TL;DR
This paper explores how stars embedded in accretion disks around supermassive black holes during AGN activation experience rapid orbital decay, leading to observable flares and tidal disruption events that depend on black hole mass and orbital orientation.
Contribution
It introduces a model of starfall during AGN turn-on, predicting observable signatures like optical/UV flares and TDEs, and links these to SMBH mass and disk dynamics.
Findings
Stars experience rapid orbital decay in AGN disks.
Flares and TDEs depend on SMBH mass and orbit orientation.
Retrograde TDEs are over-luminous and short-lived.
Abstract
As active galactic nuclei (AGN) `turn on', some stars end up embedded in accretion disks around supermassive black holes (SMBHs) on retrograde orbits. Such stars experience strong headwinds, aerodynamic drag, ablation and orbital evolution on short timescales. Loss of orbital angular momentum in the first ~Myr of an AGN leads to a heavy rain of stars (`starfall') into the inner disk and onto the SMBH. A large AGN loss cone () can result from binary scatterings in the inner disk and yield tidal disruption events (TDEs). Signatures of starfall include optical/UV flares that rise in luminosity over time, particularly in the inner disk. If the SMBH mass is , flares truncate abruptly and the star is swallowed. If , and if the infalling orbit lies within , the flare is followed…
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