activity
20162021
most citedConstraining the magnetic field in the TeV halo of Geminga with X-ray Observation

40 citations · 93 across the 5 of their papers we have counts for

collaborators

12 papers

astro-ph.GA20217 cited

The BIG X-ray tail

Chong Ge, Ming Sun, Masafumi Yagi +9

Galaxy clusters grow primarily through the continuous accretion of group-scale haloes. Group galaxies experience preprocessing during their journey into clusters. A star-bursting c…

astro-ph.GA2021

An H/X-ray orphan cloud as a signpost of the intracluster medium clumping

Chong Ge, Rongxin Luo, Ming Sun +12

Recent studies have highlighted the potential significance of intracluster medium (ICM) clumping and its important implications for cluster cosmology and baryon physics. Many of th…

astro-ph.HE2020

Revealing a peculiar supernova remnant G106.3+2.7 as a petaelectronvolt proton accelerator with X-ray observations

Chong Ge, Ruo-Yu Liu, Shu Niu +2

Supernova remnants (SNRs) have long been considered as one of the most promising sources of Galactic cosmic rays. In the SNR paradigm, petaelectronvolt (PeV) proton acceleration ma…

astro-ph.GA202016 cited

Chandra and XMM-Newton observations of A2256: cold fronts, merger shocks, and constraint on the IC emission

Chong Ge, Ruo-Yu Liu, Ming Sun +13

We present the results of deep Chandra and XMM-Newton observations of a complex merging galaxy cluster Abell 2256 (A2256) that hosts a spectacular radio relic (RR). The temperature…

astro-ph.GA2020

The ram pressure stripped radio tails of galaxies in the Coma cluster

Hao Chen, Ming Sun, Masafumi Yagi +14

Previous studies have revealed a population of galaxies in galaxy clusters with ram pressure stripped (RPS) tails of gas and embedded young stars. We observed 1.4 GHz continuum and…

astro-ph.HE202011 cited

AGN feedback in the FR II galaxy 3C 220.1

Wenhao Liu, Ming Sun, Paul E. J. Nulsen +6

We present results from a deep (174 ks) Chandra observation of the FR-II radio galaxy 3C 220.1, the central brightest cluster galaxy (BCG) of a 4 keV cluster at .…