Chandra Observation of Abell 1142: A Cool-Core Cluster Lacking a Central Brightest Cluster Galaxy?
Yuanyuan Su (1), David A. Buote (2), Fabio Gastaldello (3), Reinout, van Weeren (1) ((1) Harvard-Smithsonian Center for Astrophysics, (2) UC, Irvine, (3) INAF-IASF-Milano)

TL;DR
This study uses Chandra X-ray observations to analyze Abell 1142, revealing it as a cool-core cluster with a displaced center, ongoing subcluster merger, and complex galaxy dynamics, challenging typical BCG associations.
Contribution
It provides the first detailed X-ray analysis of Abell 1142, identifying its cool core, subcluster merger, and the displacement of the cluster center from the BCGs.
Findings
Abell 1142 has a displaced X-ray emission peak about 100 kpc from BCGs.
The cluster exhibits a cool core with higher metallicity and lower temperature.
A merger between two subclusters is ongoing, affecting the ICM and scaling relations.
Abstract
Abell~1142 is a low-mass galaxy cluster at low redshift containing two comparable Brightest Cluster Galaxies (BCG) resembling a scaled-down version of the Coma Cluster. Our Chandra analysis reveals an X-ray emission peak, roughly 100 kpc away from either BCG, which we identify as the cluster center. The emission center manifests itself as a second beta-model surface brightness component distinct from that of the cluster on larger scales. The center is also substantially cooler and more metal rich than the surrounding intracluster medium (ICM), which makes Abell 1142 appear to be a cool core cluster. The redshift distribution of its member galaxies indicates that Abell 1142 may contain two subclusters with each containing one BCG. The BCGs are merging at a relative velocity of ~1200 km/s. This ongoing merger may have shock-heated the ICM from ~ 2 keV to above 3 keV, which would explain…
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