collaborators

5 papers

astro-ph.CO2026

The Quiescent Sloshing Core of Abell 496 with XRISM

Angie Veronica, Thomas H. Reiprich, Naomi Ota +9

Gas motions provide insight into the dynamical history and physical processes within galaxy clusters. We investigate the kinematics of the ICM in the core of A496, a nearby, X-ray…

astro-ph.GA2026

Solving the cooling flow problem with combined jet-wind AGN feedback

Aoyun He, Feng Yuan, Suoqing Ji +6

Active galactic nucleus (AGN) feedback is widely viewed as the most promising solution to the long-standing cooling flow problem in galaxy clusters, yet previous models prescribe j…

astro-ph.GA2025

A Chandra view of SPT-CL J0217-5014: a massive galaxy cluster at a cosmic intersection at z=0.53

Dan Hu, Shida Fan, Zhongsheng Yuan +7

Galaxy clusters trace the densest regions of the cosmic web and are crucial laboratories for studying the thermodynamic and chemical evolution of the intracluster medium (ICM). We…

astro-ph.GA2025

The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters

Yuanyuan Zhao, Haiguang Xu, Ang Liu +8

Cosmological simulations indicate that nearly half of the baryons in the nearby Universe are in the warm-hot intergalactic medium (WHIM) phase, and about a half them reside in cosm…

astro-ph.CO2025

MeerKAT discovery of GHz radio emission extending from Abell 3017 toward Abell 3016

Dan Hu, Norbert Werner, Haiguang Xu +18

Context: The clusters Abell 3017 and Abell 3016 are located within a large-scale filament. A prominent X-ray bridge has been detected connecting the two clusters and a potential ga…