activity
20182026
most citedThe formation of dusty cold gas filaments from galaxy cluster simulations

40 citations · 188 across the 11 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026

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…

astro-ph.GA2022★ 16 cited

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…

astro-ph.GA2022★ 11 cited

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…

astro-ph.GA2021★ 11 cited

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…

astro-ph.GA2020★ 40 cited

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…

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.GA2018★ 15 cited

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…