collaborators

6 papers

astro-ph.HE2026

Metal sign of a large-scale AGN feedback in cool-core cluster MACS J1931.8-2634

Qinnan Zhu, Junjie Mao, Ping Zhou +2

The spatial distribution of metals in the intracluster medium (ICM) is a sensitive tracer of the chemical and dynamical history of galaxy clusters. While most cool-core (CC) cluste…

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.CO2025

Suzaku Observation of Merging Clusters Abell 222 and Abell 223

Yanling Chen, Wei Cui, Aurora Simionescu +2

Previous X-ray and optical studies of the galaxy cluster pair Abell 222/223 suggested the possible presence of a filamentary structure connecting the two clusters, a result that ap…

astro-ph.GA2025

MWA and VLA Observations of Diffuse Radio Lobes in M 87

Linhui Wu, Fu-Guo Xie, Qian Zheng +12

This study investigates the projected, quasi-symmetric -scale diffuse radio lobes surrounding the giant elliptical galaxy M\,87, utilizing well-sampled wideband ($\…

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…