Deep Chandra Observations of Abell 2199: the Interplay between Merger-Induced Gas Motions and Nuclear Outbursts in a Cool Core Cluster
Paul E. J. Nulsen (1), Zhiyuan Li (1, 2), William R. Forman (1), Ralph, P. Kraft (1), Dharam V. Lal (1, 3), Christine Jones (1), Irina Zhuravleva, (4), Eugene Churazov (5), Jeremy S. Sanders (6), Andrew C. Fabian (7), Ryan, E. Johnson (8), Stephen S. Murray (9) ((1) CfA

TL;DR
This study uses Chandra X-ray observations to explore gas motions, shocks, and radio interactions in the cool core cluster Abell 2199, revealing complex merger-induced phenomena and AGN activity effects.
Contribution
First detailed analysis linking merger-induced gas sloshing, shocks, and AGN radio outbursts in Abell 2199 using deep Chandra data.
Findings
Evidence of gas sloshing from a minor merger about 400 Myr ago.
Detection of a Mach 1.46 shock with no clear temperature jump.
Discrepancy between shock energy and radio lobe enthalpy suggests recent, less powerful AGN activity.
Abstract
We present new Chandra observations of Abell 2199 that show evidence of gas sloshing due to a minor merger, as well as impacts of the radio source, 3C 338, hosted by the central galaxy, NGC 6166, on the intracluster gas. The new data are consistent with previous evidence of a Mach 1.46 shock 100" from the cluster center, although there is still no convincing evidence for the expected temperature jump. Other interpretations of this feature are possible, but none is fully satisfactory. Large scale asymmetries, including enhanced X-ray emission 200" southwest of the cluster center and a plume of low entropy, enriched gas reaching 50" to the north of the center, are signatures of gas sloshing induced by core passage of a merging subcluster about 400 Myr ago. An association between the unusual radio ridge and low entropy gas are consistent with this feature being the remnant of a former…
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