40 citations · 188 across the 11 of their papers we have counts for
11 papers
Satellite quenching by radio jets of central galaxies in galaxy groups
Yijun Wang, Tao Wang, Dingyi Zhao +9
Feedback from active galactic nuclei (AGN) is now recognized as a key component of galaxy formation models. It plays a central role in regulating the growth and quenching of galaxi…
Predictions of and neutrino mass from a consistent Froggatt-Nielsen model
Yu-Cheng Qiu, Jin-Wei Wang, Tsutomu T. Yanagida
The seesaw mechanism is the most attractive mechanism to explain the small neutrino masses, which predicts the neutrinoless double beta decay () of the nucleus. Thus the disc…
Radio jet-ISM interaction and positive radio-mechanical feedback in Abell 1795
Prathamesh D. Tamhane, Brian R. McNamara, Helen R. Russell +8
We present XSHOOTER observations with previous ALMA, MUSE and observations to study the nature of radio-jet triggered star formation and the interaction of radio jets with th…
A Novel Solution to the Gravitino Problem
Yu-Cheng Qiu, S. -H. Henry Tye
In a general phenomenological model with local supersymmetry, the amount of massive gravitinos produced in early universe tends to violate the known dark matter density bound by ma…
Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven H Filaments
Haojie Hu, Yu Qiu, Marie-Lou Gendron-Marsolais +5
The hot intracluster medium (ICM) is thought to be quiescent with low observed velocity dispersions. Surface brightness fluctuations of the ICM also suggest that its turbulence is…
Milli-Hertz Gravitational Wave Background Produced by Quasi-Periodic Eruptions
Xian Chen, Yu Qiu, Shuo Li +1
Extreme-mass-ratio inspirals (EMRIs) are important targets for future space-borne gravitational-wave (GW) detectors, such as the Laser Interferometer Sapce Antenna (LISA). Recent w…
Magnetic Twists of Solar Filaments
Jinhan Guo, Yiwei Ni, Ye Qiu +3
Solar filaments are cold and dense materials situated in magnetic dips, which show distinct radiation characteristics compared to the surrounding coronal plasma. They are associate…
On the Mass Loading of AGN-Driven Outflows in Elliptical Galaxies and Clusters
Yu Qiu, Brian R. McNamara, Tamara Bogdanovic +2
Outflows driven by active galactic nuclei (AGN) are an important channel for accreting supermassive black holes (SMBHs) to interact with their host galaxies and clusters. Propertie…
The formation of dusty cold gas filaments from galaxy cluster simulations
Yu Qiu, Tamara Bogdanovic, Yuan Li +2
Galaxy clusters are the most massive collapsed structures in the universe whose potential wells are filled with hot, X-ray emitting intracluster medium. Observations however show t…
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…
Using H Filaments to Probe AGN Feedback in Galaxy Clusters
Yu Qiu, Tamara Bogdanovic, Yuan Li +1
Recent observations of giant ellipticals and brightest cluster galaxies (BCGs) provide tentative evidence for a correlation between the luminosity of the H emitting gas filament…