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20102026
most citedAssisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"

512 citations · 5.2k across the 67 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.GA2017★ 100 cited

Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem

Taeho Ryu, Rosalba Perna, Zoltán Haiman +2

Using few-body simulations, we investigate the evolution of supermassive black holes (SMBHs) in galaxies ( at ) at . Following…

astro-ph.GA2017★ 65 cited

The Delay Time Distribution of Tidal Disruption Flares

Nicholas C. Stone, Aleksey Generozov, Eugene Vasiliev +1

Recent observations suggest that stellar tidal disruption events (TDE) are strongly overrepresented in rare, post-starburst galaxies. Several dynamical mechanisms have been propose…

astro-ph.GA2017★ 160 cited

Black hole masses of tidal disruption event host galaxies

Thomas Wevers, Sjoert van Velzen, Peter G. Jonker +5

The mass of the central black hole in a galaxy that hosted a tidal disruption event (TDE) is an important parameter in understanding its energetics and dynamics. We present the fir…

astro-ph.HE2017★ 36 cited

Periodic accretion-powered flares from colliding EMRIs as TDE Imposters

Brian D. Metzger, Nicholas C. Stone

When a main sequence star undergoes Roche lobe overflow onto a supermassive black hole (SMBH) in a circular extreme mass ratio inspiral (EMRI), a phase of steady mass transfer ensu…

astro-ph.HE2017★ 36 cited

Optical/UV-to-X-Ray Echoes from the Tidal Disruption Flare ASASSN-14li

Dheeraj R. Pasham, S. Bradley Cenko, Aleksander Sadowski +4

We carried out the first multi-wavelength (optical/UV and X-ray) photometric reverberation mapping of a tidal disruption flare (TDF) ASASSN-14li. We find that its X-ray variations…

astro-ph.HE2017★ 67 cited

Gravitational-Wave Localization Alone Probes AGN Origin of Stellar-Mass Black Hole Mergers

I. Bartos, Z. Haiman, Z. Marka +3

Stellar-mass binary black hole mergers are poised to represent the majority of gravitational-wave (GW) observations by Advanced LIGO and Virgo. Probing their origin will be difficu…