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Abell 223

From Wikipedia, the free encyclopedia
Galaxy cluster in the constellation Cetus

Abell 223
Observation data (EpochJ2000)
ConstellationCetus
Right ascension01h 37m 55.9s[1]
Declination−12° 49′ 11″[1]
Brightest memberLEDA 947139[2]
Richness class3[3]
Bautz–Morgan classificationIII[3]
Velocity dispersion1,032 km/s[4]
Redshift0.2079 ± 0.0008[4]
Distance2.4 Gly (740 Mpc)[5]
ICM temperature4.38 ± 0.16[4]
Other designations
RXC J0137.9-1248[1]

Abell 223 is agalaxy cluster. It is located at a distance of 2.4 billion light-years fromEarth.The cluster is connected to nearby clusterAbell 222 by a filament of matter. Research has shown that only 20% of that matter is normal. The rest is thought to be dark matter.[5] This means that this would form theAbell 222/ Abell 223Supercluster as we understand them.[6]

See also

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References

[edit]
  1. ^abc"ACO 223".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved26 November 2017.
  2. ^"2MASX J01375602-1249106".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved26 November 2017.
  3. ^abAbell, George O.; Corwin, Harold G. Jr.; Olowin, Ronald P. (May 1989)."A catalog of rich clusters of galaxies".Astrophysical Journal Supplement Series.70 (May 1989):1–138.Bibcode:1989ApJS...70....1A.doi:10.1086/191333.ISSN 0067-0049.
  4. ^abcDurret, F; Laganá, T. F; Adami, C; Bertin, E (2010). "The clusters Abell 222 and Abell 223: A multi-wavelength view".Astronomy and Astrophysics.517: A94.arXiv:1005.3295.Bibcode:2010A&A...517A..94D.doi:10.1051/0004-6361/201014566.S2CID 118464154.
  5. ^abPete Spotts (5 July 2012)."Cosmic scaffolding uncovered? Scientists find thread of dark matter".The Christian Science Monitor.Christian Science Publishing Society. Retrieved14 July 2012.
  6. ^Dietrich, Jörg."The Abell 222/223 Supercluster with dark matter Filament". University of Michigan/University Observatory Munich. Retrieved24 June 2020.
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