Khác biệt giữa bản sửa đổi của “Siêu đám thiên hà”
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n →Các siêu đám cực xa: sửa chính tả 2, replaced: . → . using AWB |
n fixes, replaced: cite → chú thích (10), → |
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Dòng 24:
| It contains the [[Local Group]] with our [[galaxy]], the [[Milky Way]]. It also contains the [[Virgo Cluster]] near its center, and is sometimes called the Local Supercluster. It is thought to contain over 47,000 galaxies.
In 2014, the newly announced [[Laniakea Supercluster]] subsumed the Virgo Supercluster, which became a component of the new supercluster.<ref name=2014arXiv1409.0880T>{{
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| [[Siêu đám Trường Xà–Bán Nhân Mã]] (''{{lang|en|Hydra-Centaurus Supercluster}}'')
Dòng 65:
* 18 Mpc x 26 Mpc
| Forming the far wall of the [[Ophiuchus Void]], it may be connected in a filament, with the [[Pavo-Indus-Telescopium Supercluster]] and the [[Hercules Supercluster]]. This supercluster is centered on the cD cluster [[Ophiuchus Cluster]], and has at least two more galaxy clusters, four more galaxy groups, several field galaxies, as members.<ref>
{{
|author=Hasegawa, T. ''et al.''
|date=2000
Dòng 104:
| [[Siêu đám Bắc Miện]] (''{{lang|en|Corona Borealis Supercluster}}'')
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:[[Redshift|z]]=0.07<ref name=postman88>{{
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Dòng 199:
| [[Redshift|z]]=1.27
| Discovered in 1999<ref>
{{
|author=Rosati, P. ''et al''
|date=1999
Dòng 214:
|work=[[SIMBAD]]
}}</ref> it contains at least two clusters [[RXJ 0848.9+4452]] (z=1.26) and [[RXJ 0848.6+4453]] (z=1.27). At the time of discovery, it became the most distant known supercluster.<ref>
{{
|author=Nakata, F. ''et al.''
|date=2004
Dòng 225:
|isbn=0-521-84908-X
}}</ref> Additionally, seven smaller groups of galaxies are associated with the supercluster.<ref>
{{
|author=Ohta, K. ''et al.''
|date=2003
Dòng 242:
Length=70Mpc
| A rich supercluster with several galaxy clusters was discovered around an unusual concentration of 23 [[quasar|QSO]]s at z=1.1 in 2001. The size of the complex of clusters may indicate a [[galaxy filament|wall of galaxies]] exists there, instead of a single supercluster. The size discovered approaches the size of the [[CfA2 Great Wall]] filament. At the time of the discovery, it was the largest and most distant supercluster beyond z=0.5 <ref>
{{
|author=Tanaka, I.
|date=2004
Dòng 250:
|bibcode=2004sgyu.conf...61T
}}</ref><ref>
{{
|author=Tanaka, I.; Yamada, T.; Turner, E. L.; Suto, Y.
|date=2001
Dòng 263:
| SCL @ 1604+43 at z=0.9
| [[Redshift|z]]=0.91
| This supercluster at the time of its discovery was the largest supercluster found so deep into space, in 2000. It consisted of two known rich clusters and one newly discovered cluster as a result of the study that discovered it. The then known clusters were [[Cl 1604+4304]] (z=0.897) and [[Cl 1604+4321]] (z=0.924), which then known to have 21 and 42 known galaxies respectively. The then newly discovered cluster was located at {{RA|16|04|25.7}}, {{DEC|+43|14|44.7}}<ref>{{
|title=A Definitive Optical Detection of a Supercluster at [CLC][ITAL]z[/ITAL][/CLC] ≈ 0.91
|date=2000
Dòng 284:
| [[Redshift|z]]=0.54
| This supercluster lies around radio galaxy [[54W084C]] (z=0.544) and is composed of at least three large clusters, [[CL 0016+16]] (z=0.5455), [[RX J0018.3+1618]] (z=0.5506), [[RX J0018.8+1602]].<ref>
{{
|title=Superclustering at Redshift [CLC][ITAL]z[/ITAL] = 0.54[/CLC]
|date=1996
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