2011A&A...527A..21B


C.D.S. - SIMBAD4 rel 1.7 - 2019.10.21CEST00:39:51

2011A&A...527A..21B - Astronomy and Astrophysics, volume 527A, 21-21 (2011/3-1)

A2163: merger events in the hottest Abell galaxy cluster. II. Subcluster accretion with galaxy-gas separation.

BOURDIN H., ARNAUD M., MAZZOTTA P., PRATT G.W., SAUVAGEOT J.-L., MARTINO R., MAUROGORDATO S., CAPPI A., FERRARI C. and BENOIST C.

Abstract (from CDS):

Located at z=0.203, A2163 is a rich galaxy cluster with an intra-cluster medium (ICM) that exhibits extraordinary properties, including an exceptionally high X-ray luminosity, average temperature, and a powerful and extended radio halo. The irregular and complex morphology of its gas and galaxy structure suggests that this cluster has recently undergone major merger events that involve two or more cluster components. In this paper, we study the gas structure and dynamics by means of spectral-imaging analysis of X-ray data obtained from XMM-Newton and Chandra observations. From the evidence of a cold front, we infer the westward motion of a cool core across the E-W elongated atmosphere of the main cluster A2163-A. Located close to a galaxy over-density, this gas ``bullet'' appears to have been spatially separated from its galaxy (and presumably dark matter component) as a result of high-velocity accretion. From gas brightness and temperature profile analysis performed in two opposite regions of the main cluster, we show that the ICM has been adiabatically compressed behind the crossing ``bullet'' possibly because of shock heating, leading to a strong departure of the ICM from hydrostatic equilibrium in this region. Assuming that the mass estimated from the YX proxy best indicates the overall mass of the system and that the western cluster sector is in approximate hydrostatic equilibrium before subcluster accretion, we infer a merger scenario between two subunits of mass ratio 1:4, leading to a present total system mass of M500≃1.9x1015M. Additional analysis of the spatially-separated northern subcluster A2163-B does not show any evidence of strong interaction with the main cluster A2163-A, leading us to infer that the physical distance separating the northern subcluster and the main component is longer than the projected separation of these components. The exceptional properties of A2163 present various similarities with those of 1E0657-56, the so-called ``bullet-cluster''. These similarities are likely to be related to a comparable merger scenario.

Abstract Copyright:

Journal keyword(s): galaxies: clusters: general - intergalactic medium - X-rays: galaxies: clusters

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 ClG 0657-56 ClG 06 58 29.6 -55 56 39           ~ 774 1
2 NAME North Polar Spur ISM 12 00 +00.0           ~ 297 1
3 ACO 2163 ClG 16 15 34.1 -06 07 26           ~ 512 0
4 NAME LHB X 16 42.0 +02 19           ~ 240 0

    Equat.    Gal    SGal    Ecl

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2019.10.21-00:39:51

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