Editing Centaurus Cluster (section)

{{Short description|Galaxy cluster in the constellation Centaurus}}
{{distinguish|Hydra–Centaurus Supercluster|Centaurus A/M83 Group}}

{{Infobox galaxy cluster 
| name = Centaurus Cluster
| image = File:NGC 4706 NGC 4709 legacy dr10.jpg
| caption= 
| constellation = [[Centaurus]]
| epoch = [[Epoch (astronomy)#Julian years and J2000|J2000]]
| ra = {{RA|12|48|51.8}}<ref name="NED">{{cite web
  | title=NASA/IPAC Extragalactic Database
  | work=Results for Centaurus Cluster
  | url=http://nedwww.ipac.caltech.edu/
  | access-date=2006-10-19}}</ref>
| dec = {{DEC|-41|18|21}}<ref name="NED"/>
| redshift = 0.01140 (3 418 km/s)<ref name="NED"/>
| member_no = ~100<ref name="NED"/>
| richness = 0<ref name="ACO">{{cite journal
 | last1 = Abell
 | first1 = George O.
 | author-link1 = George O. Abell
 | last2 = Corwin
 | first2 = Harold G. Jr.
 | author-link2 = Harold G. Corwin
 | last3 = Olowin
 | first3 = Ronald P.
 | author-link3 = Ronald P. Olowin
 |date=May 1989
 | title = A catalog of rich clusters of galaxies
 | journal = Astrophysical Journal Supplement Series
 | volume = 70
 | issue = May 1989
 | pages = 1–138
 | issn = 0067-0049
 | bibcode = 1989ApJS...70....1A
 | doi = 10.1086/191333
 | doi-access = free
 }}</ref>
| bmtype = I–II <ref name="ACO" />
| brightest_member = [[NGC 4696]]
| velocity_dispersion = 
| distance = {{convert|52.4|Mpc|Mly|1|abbr=on|lk=on}} {{hub|0.705}}<ref name="NED" />
| temperature = 
| mass = <!-- 0{{e|14}} {{hub|0.00}} [[solar mass|M<sub>☉</sub>]] -->
| luminosity = 
| flux = 15.7{{e|-11}} [[erg]] s<sup>−1</sup> cm<sup>−2</sup> (0.5–2 [[electron volt|keV]]) <ref name="NED" />
| other_names = [[Abell catalogue|Abell]] 3526<ref name="NED"/>
}} 
The '''Centaurus Cluster''' (A3526) is a [[Groups and clusters of galaxies|cluster]] of hundreds of [[galaxy|galaxies]], located approximately 170 million [[light-year]]s away in the [[Centaurus]] constellation.  The brightest member galaxy is the [[elliptical galaxy]] [[NGC 4696]] (~11m). The Centaurus cluster shares its supercluster, the [[Hydra–Centaurus Supercluster]], with [[IC4329 Cluster]] and [[Hydra Cluster]].

The cluster consists of two different sub-groups of galaxies with different velocities.<ref name=":0">{{cite journal | bibcode = 1986MNRAS.221..453L | title=The Centaurus cluster of galaxies. II – The bimodal velocity structure | journal=Monthly Notices of the Royal Astronomical Society | volume=221 | pages=453–472 | year=1986| author=Lucey J. R.| author2=Currie M. J.| author3=Dickens R. J. | issue=2 | doi=10.1093/mnras/221.2.453| doi-access=free }}</ref> Cen 30 is the main subgroup containing [[NGC 4696]]. Cen 45 which is centered on [[NGC 4709]], is moving at 1500&nbsp;km/s relative to Cen 30,<ref name=":0" /> and is believed to be merging with the main cluster.<ref>{{Cite journal|last1=Churazov|first1=E.|last2=Gilfanov|first2=M.|last3=Forman|first3=W.|last4=Jones|first4=C.|date=1999|title=Evidence for Merging in the Centaurus Cluster|url=http://stacks.iop.org/0004-637X/520/i=1/a=105|journal=The Astrophysical Journal|language=en|volume=520|issue=1|page=105|doi=10.1086/307421|issn=0004-637X|arxiv=astro-ph/9802166|bibcode=1999ApJ...520..105C|s2cid=18552647 }}</ref>