SIMBAD references

2016ApJ...821...40S - Astrophys. J., 821, 40-40 (2016/April-2)

Chandra observation of Abell 1142: a cool-core cluster lacking a central brightest cluster galaxy?

SU Y., BUOTE D.A., GASTALDELLO F. and VAN WEEREN R.

Abstract (from CDS):

Abell 1142 is a low-mass galaxy cluster at low redshift containing two comparable brightest cluster galaxies (BCGs) 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, each of which contain one BCG. The BCGs are merging at a relative velocity of ≃1200 km s-1. This ongoing merger may have shock-heated the ICM from ≃2 keV to above 3 keV, which would explain the anomalous LX-TX scaling relation for this system. This merger may have displaced the metal-enriched "cool core" of either of the subclusters from the BCG. The southern BCG consists of three individual galaxies residing within a radius of 5 kpc in projection. These galaxies should rapidly sink into the subcluster center due to the dynamical friction of a cuspy cold dark matter halo.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): dark matter - galaxies: clusters: individual: Abell 1142 - galaxies: clusters: intracluster medium - galaxies: individual: (NGC 3492, IC 664) - galaxies: ISM

Simbad objects: 15

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2019.12.10-03:31:31

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