activity
20122026
most citedDescope of the ALIA mission

146 citations · 656 across the 21 of their papers we have counts for

collaborators
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.GA2022★ 21 cited

Revisit the rate of tidal disruption events: the role of the partial tidal disruption event

Shiyan Zhong, Shuo Li, Peter Berczik +1

Tidal disruption of stars in dense nuclear star clusters containing supermassive central black holes (SMBH) is modeled by high-accuracy direct N-body simulation. Stars getting too…

astro-ph.GA2019★ 18 cited

Direct n-body simulations of tidal disruption rate evolution in unequal-mass galaxy mergers

Shuo Li, Peter Berczik, Xian Chen +3

The hierarchical galaxy formation model predicts supermassive black hole binaries (SMBHBs) in galactic nuclei. Due to the gas poor environment and the limited spatial resolution in…

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.GA2014★ 8 cited

Star cluster disruption in the starburst galaxy Messier 82

Shuo Li, Richard de Grijs, Peter Anders +1

Using high-resolution, multiple-passband Hubble Space Telescope images spanning the entire optical/near-infrared wavelength range, we obtained a statistically complete sample, -…

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…