Showing 1–20 of 27 results
/ Date/ Name
Aug 31, 2020Extracting the Possible Intrinsic Relation between Radiative Efficiency and Mass of QSOs: a Maximum Likelihood Method and its Application to the SDSS DR7 QSOsMar 15, 2017On the post-Keplerian corrections to the orbital periods of a two-body system and their application to the Galactic CenterMay 5, 2025The Secular Periodic Evolution of X-ray Quasi-periodic Eruptions Driven by Star-disc CollisionsJan 9, 2025Self-consistent Solutions of Evolving Nuclear Star Clusters with Two-Dimensional Monte-Carlo Dynamical SimulationsOct 21, 2021X-ray Quasi-periodic Eruptions driven by Star-Disc Collisions : Application to GSN069 and Probing the Spin of Massive Black HolesSep 30, 2021The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave ObservatoriesSep 25, 2017Probing the spinning of the massive black hole in the Galactic Center via pulsar timing: A Full Relativistic TreatmentMar 7, 2019Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black hole in a galactic nucleusOct 31, 2016On the Newtonian and Spin-induced Perturbations felt by the Stars Orbiting around the Massive Black Hole in the Galactic CenterOct 12, 2025Co-evolution of Nuclear Star Clusters and Massive Black Holes: Extreme Mass-Ratio InspiralsOct 19, 2009On the spatial distribution and the origin of hypervelocity starsMay 7, 2011The spatial and velocity distributions of hypervelocity starsNov 10, 2023A centi-pc-scale compact radio core in the nearby galaxy M60Feb 11, 2014On the Existence of Pulsars in the Vicinity of the Massive Black Hole in the Galactic CenterNov 8, 2021Impact of cosmic filaments on the gas accretion rate of dark matter halosSep 18, 2024Improving constraints on the extended mass distribution in the Galactic Center with stellar orbitsOct 4, 2017Evidence for higher black hole spin in radio-loud quasarsAug 17, 2018The scattering of FRBs by the intergalactic medium: variations, strength and dependence on dispersion measuresDec 4, 2023Prospects for probing small-scale dark matter models with pulsars around Sagittarius A*Jul 19, 2021Profiles of cosmic filaments since z=4.0 in cosmological hydrodynamical simulation