35 citations · 59 across the 9 of their papers we have counts for
7 papers · 1 filter
A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications
Yuan Wang, Xiong Luo, Huiyuan Wang +5
Precession is a very common phenomenon for small-scale astronomical objects. However, the precession of galactic disks, occurring on a scale larger than kilo-parsec, has barely bee…
Radio AGN feedback sustains quiescence only in a minority of massive galaxies
Huiling Liu, Yan Lu, Hui Hong +11
Radio active galactic nuclei (AGNs) eject a huge amount of energy into the surrounding medium and are thought to potentially prevent gas cooling and maintain the quiescence of mass…
Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
Hao Li, Yangyao Chen, Huiyuan Wang +1
We explore the co-evolution of dark matter halos, their central galaxies, and central supermassive black holes (SMBHs) using the IllustrisTNG (TNG) simulation. We find that the evo…
ELUCID VIII: Simulating the Coma Galaxy Cluster to Calibrate Model and Understand Feedback
Xiong Luo, Huiyuan Wang, Weiguang Cui +9
We conducted an investigation of the Coma cluster of galaxies by running a series of constrained hydrodynamic simulations with GIZMO-SIMBA and GADGET-3, based on initial conditions…
Halo mass-observable proxy scaling relations and their dependencies on galaxy and group properties
Ziwen Zhang, Huiyuan Wang, Wentao Luo +5
Based on the DECaLS shear catalog, we study the scaling relations between halo mass() and various proxies for SDSS central galaxies, including stellar mass(), stell…
Shock-induced stripping of satellite ISM/CGM in IllustrisTNG clusters at
Hao Li, Huiyuan Wang, H. J. Mo +3
Using the IllustrisTNG simulation, we study the interaction of large-scale shocks with the circumgalactic medium (CGM) and interstellar medium (ISM) of star-forming (SF) satellite…
Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
Ziwen Zhang, Huiyuan Wang, Wentao Luo +5
In the local Universe, the efficiency for converting baryonic gas into stars is very low. In dark matter halos where galaxies form and evolve, the average efficiency varies with ga…