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Abell 2163

Abell 2163 is one of the richest and most distant of the clusters of galaxies found in the Abell catalogue. Its abell richness class is 2 and position is at a redshift z=0.2. Data from Chandra X-ray Observatory have shown that it is the hottest galaxy cluster in the Abell catalogue. It is also a merging cluster.

Abell 2163
Abell 2163 taken by Hubble Space Telescope.[1]
Observation data (Epoch J2000)
Constellation(s)Ophiuchus
Right ascension16h 15m 34.1s
Declination−06° 07′ 26.04″
Richness class2[2]
Redshift0.2030[3]
Distance828 Mpc (2,701 Mly) h−1
0.705
[3]
ICM temperature11.5–14.6 keV
Binding mass4.6 × 1015 M
X-ray luminosity6 × 1045erg/s
X-ray flux1.4×10−11 erg s−1 cm−2 (0.5–2 keV) [3]
See also: Galaxy group, Galaxy cluster, List of galaxy groups and clusters

The galaxy density and mass distribution in the central region of this cluster have also been determined by weak gravitational lensing. These analyses show very similar mass and galaxy distributions, with two coincident maxima and a flat shape elongated in the east-west direction, but the weak lensing signal is surprisingly faint in comparison to what could be expected from the cluster X-ray properties. However, these detailed studies are limited to the inner 8’×8’ region of the cluster, and do not include the peripheral clumps such as A2163-B. La Barbera et al. (2004) estimated the photometric redshifts of galaxies in A2163-B, showing that this structure lies at the typical redshift of the main cluster (z = 0.215 ± 0.0125).[4]

There is also an extremely bright and large radio halo present in the cluster, and is one of the brightest known clusters.[5]

See also edit

References edit

  1. ^ "Cosmic fireflies". www.spacetelescope.org. Retrieved 11 December 2017.
  2. ^ Abell, George O.; Corwin, Harold G., Jr.; Olowin, Ronald P. (May 1989). "A catalog of rich clusters of galaxies" (PDF). Astrophysical Journal Supplement Series. 70 (May 1989): 1–138. Bibcode:1989ApJS...70....1A. doi:10.1086/191333. ISSN 0067-0049. Retrieved March 13, 2012.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  3. ^ a b c "NED results for object ABELL 2163". NASA/IPAC Extragalactic Database (NED). Retrieved March 17, 2012.
  4. ^ A2163: Merger events in the hottest Abell galaxy cluster I. Dynamical analysis from optical data – S.Maurogordato, A. Cappi, C. Ferrari, C. Benoist, G. Mars, G. Soucail, M. Arnaud, G.W. Pratt, H. Bourdin, J.-L. Sauvageot.
  5. ^ The Giant Radio Halo in Abell 2163 – L. Feretti, R. Fusco-Femiano, G. Giovannini, F. Govoni.


abell, 2163, richest, most, distant, clusters, galaxies, found, abell, catalogue, abell, richness, class, position, redshift, data, from, chandra, observatory, have, shown, that, hottest, galaxy, cluster, abell, catalogue, also, merging, cluster, taken, hubble. Abell 2163 is one of the richest and most distant of the clusters of galaxies found in the Abell catalogue Its abell richness class is 2 and position is at a redshift z 0 2 Data from Chandra X ray Observatory have shown that it is the hottest galaxy cluster in the Abell catalogue It is also a merging cluster Abell 2163Abell 2163 taken by Hubble Space Telescope 1 Observation data Epoch J2000 Constellation s OphiuchusRight ascension16h 15m 34 1sDeclination 06 07 26 04 Richness class2 2 Redshift0 2030 3 Distance828 Mpc 2 701 Mly h 10 705 3 ICM temperature11 5 14 6 keVBinding mass4 6 1015 M X ray luminosity6 1045erg sX ray flux1 4 10 11 erg s 1 cm 2 0 5 2 keV 3 See also Galaxy group Galaxy cluster List of galaxy groups and clustersThe galaxy density and mass distribution in the central region of this cluster have also been determined by weak gravitational lensing These analyses show very similar mass and galaxy distributions with two coincident maxima and a flat shape elongated in the east west direction but the weak lensing signal is surprisingly faint in comparison to what could be expected from the cluster X ray properties However these detailed studies are limited to the inner 8 8 region of the cluster and do not include the peripheral clumps such as A2163 B La Barbera et al 2004 estimated the photometric redshifts of galaxies in A2163 B showing that this structure lies at the typical redshift of the main cluster z 0 215 0 0125 4 There is also an extremely bright and large radio halo present in the cluster and is one of the brightest known clusters 5 See also editAbell catalogue List of Abell clusters X ray astronomyReferences edit Cosmic fireflies www spacetelescope org Retrieved 11 December 2017 Abell George O Corwin Harold G Jr Olowin Ronald P May 1989 A catalog of rich clusters of galaxies PDF Astrophysical Journal Supplement Series 70 May 1989 1 138 Bibcode 1989ApJS 70 1A doi 10 1086 191333 ISSN 0067 0049 Retrieved March 13 2012 a href Template Cite journal html title Template Cite journal cite journal a CS1 maint multiple names authors list link a b c NED results for object ABELL 2163 NASA IPAC Extragalactic Database NED Retrieved March 17 2012 A2163 Merger events in the hottest Abell galaxy cluster I Dynamical analysis from optical data S Maurogordato A Cappi C Ferrari C Benoist G Mars G Soucail M Arnaud G W Pratt H Bourdin J L Sauvageot The Giant Radio Halo in Abell 2163 L Feretti R Fusco Femiano G Giovannini F Govoni Retrieved from https en wikipedia org w index php title Abell 2163 amp oldid 1179546228, wikipedia, wiki, book, books, library,

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