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19952026
most citedEnhanced tidal disruption rates from massive black hole binaries

144 citations · 913 across the 22 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2026

A model for the enhanced production rate of early-type hypervelocity stars in the Galactic halo

Chunyang Cao, F. K. Liu, Xian Chen +1

About twenty late B-type hypervelocity stars (HVSs) traveling faster than the Galactic escape velocity have been discovered in the Galactic halo, many of which were ejected from th…

astro-ph.GA2016★ 1 cited

Growth of supermassive black holes, galaxy mergers and supermassive binary black holes

S. Komossa, J. G. Baker, F. K. Liu

The study of galaxy mergers and supermassive binary black holes (SMBBHs) is central to our understanding of the galaxy and black hole assembly and (co-)evolution at the epoch of st…

astro-ph.GA2015★ 40 cited

Boosted Tidal Disruption by Massive Black Hole Binaries During Galaxy Mergers FROM The View of N-Body Simulation

Shuo Li, F. K. Liu, Peter Berczik +1

Supermassive black hole binaries (SMBHBs) are productions of the hierarchical galaxy formation model. There are many close connections between central SMBH and its host galaxy beca…

astro-ph.GA2012★ 28 cited

Is there an intermediate massive black hole in the Galactic center: Imprints on the stellar tidal-disruption rate

Xian Chen, F. K. Liu

It has been suggested that an intermediate-massive black hole (IMBH) with mass could fall into the galactic center (GC) and form a massive black hole binary (MBH…

astro-ph.GA2012★ 42 cited

Interaction of Recoiling Supermassive Black Holes with Stars in Galactic Nuclei

Shuo Li, F. K. Liu, Peter Berczik +2

Supermassive black hole binaries (SMBHBs) are the products of frequent galaxy mergers. The coalescence of the SMBHBs is a distinct source of gravitational wave (GW) radiation. The…

astro-ph.GA2009★ 144 cited

Enhanced tidal disruption rates from massive black hole binaries

X. Chen, P. Madau, A. Sesana +1

"Hard" massive black hole (MBH) binaries embedded in steep stellar cusps can shrink via three-body slingshot interactions. We show that this process will inevitably be accompanied…