activity
19952023
most citedA direct empirical proof of the existence of dark matter

2.4k citations · 10.9k across the 142 of their papers we have counts for

collaborators
Showing 2022 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2022★ 14 cited

Gas sloshing and cold fronts in pre-merging galaxy cluster Abell 98

Arnab Sarkar, Scott Randall, Yuanyuan Su +10

We present deep Chandra observations of the pre-merger galaxy cluster Abell 98. Abell 98 is a complex merging system. While the northern (A98N) and central subclusters (A98S) are m…

astro-ph.GA2022★ 22 cited

Discovery of a pre-merger shock in an intercluster filament in Abell 98

Arnab Sarkar, Scott Randall, Yuanyuan Su +11

We report the first unambiguous detection of an axial merger shock in the early-stage merging cluster Abell 98 using deep (227 ks) Chandra observations. The shock is about 420 kpc…

astro-ph.GA2022★ 5 cited

Resilience of Sloshing Cold Fronts against Subsequent Minor Mergers

Iraj Vaezzadeh, Elke Roediger, Claire Cashmore +8

Minor mergers are common in galaxy clusters. They have the potential to create sloshing cold fronts (SCFs) in the intracluster medium (ICM) of the cluster. However, the resilience…

astro-ph.GA2022★ 3 cited

Testing galaxy feedback models with the first resolved profiles of the circumgalactic medium

Urmila Chadayammuri, Akos Bogdan, Benjamin Oppenheimer +3

The hot ( K) phase of the circumgalactic medium (CGM) contains a large fraction of baryons in galaxies. It also retains signatures of the processes that shaped the galaxies,…

astro-ph.GA2022★ 5 cited

Chandra view of Abell 407: the central compact group of galaxies and the interaction between the radio AGN and the ICM

Chao Geng, Chong Ge, Dharam V. Lal +8

Abell 407 (A407) is a unique galaxy cluster hosting a central compact group of nine galaxies (named as 'Zwicky's Nonet'; G1 - G9 in this work) within a 30 kpc radius region. The cl…

astro-ph.GA2022

Detection of a Superluminous Spiral Galaxy in the Heart of a Massive Galaxy Cluster

Akos Bogdan, Lorenzo Lovisari, Patrick Ogle +5

It is well established that brightest cluster galaxies (BCGs), residing in the center of galaxy clusters, are typically massive and quenched galaxies with cD or elliptical morpholo…