activity
20012026
most citedChandra observtaion of A2256 - a cluster at the early stage of merging

97 citations · 403 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

Early Results from the Coma Legacy IFU Survey (CLIFS): Ram Pressure Induced Shocks and Ionization in Jellyfish Tails

Lauren M. Foster, Ian D. Roberts, Laura C. Parker +6

Jellyfish galaxies, which exhibit tails of gas opposite to their direction of motion, are a galaxy population showcasing the most extreme effects of ram pressure stripping (RPS). W…

astro-ph.HE2025★ 43 cited

The bulk motion of gas in the core of the Centaurus galaxy cluster

XRISM collaboration

Galaxy clusters, the largest gravitationally bound structures in the Universe, contain vast amounts of dark matter, galaxies, and hot ionised gas known as the intracluster medium (…

astro-ph.GA2023★ 3 cited

Exploring chemical enrichment of the intracluster medium with the Line Emission Mapper

François Mernier, Yuanyuan Su, Maxim Markevitch +27

Synthesized in the cores of stars and supernovae, most metals disperse over cosmic scales and are ultimately deposited well outside the gravitational potential of their host galaxi…

astro-ph2004★ 70 cited

Revealing the interaction between the X-ray gas of starburst galaxy UGC 6697 and the hot intracluster medium of A1367

M. Sun, A. Vikhlinin

We present the result from a CHANDRA observation of an X-ray luminous starburst galaxy UGC 6697, which is embedded in the northwest hot region of A1367 (5 - 6 keV). A very sharp X-…

astro-ph2004★ 76 cited

ESO 3060170 -- a massive fossil galaxy group with a heated gas core?

M. Sun, W. Forman, A. Vikhlinin +3

We present a detailed study of the ESO 3060170 galaxy group combining Chandra, XMM and optical observations. The system is found to be a fossil galaxy group. The group X-ray emissi…

astro-ph2002★ 53 cited

Chandra observations of the galaxy cluster A478: the interaction of hot gas and radio plasma in the core, and an improved determination of the Compton y-parameter

M. Sun, C. Jones, S. S. Murray +3

We present the results from a 42 ks \chandra ACIS observation of the galaxy cluster A478. This cluster is generally considered to be highly relaxed. The \chandra image reveals, for…