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Siêu_đám_thiên_hà
| Siêu đám thiên hà | Thông tin | Ghi chú |
|---|---|---|
| Siêu đám Laniākea (Laniakea Supercluster) |
| The Laniakea Supercluster is the supercluster that contains the Virgo Cluster, Local Group, and by extension on the latter, our galaxy; the Milky Way.[1] |
| Siêu đám Xử Nữ (Virgo Supercluster) |
| 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.[2] |
| Siêu đám Trường Xà–Bán Nhân Mã (Hydra-Centaurus Supercluster) | It is composed of two lobes, sometimes also referred to as superclusters, or sometimes the entire supercluster is referred to by these other two names
In 2014, the newly announced Laniakea Supercluster subsumed the Hydra-Centaurus Supercluster, which became a component of the new supercluster.[2] | |
| Siêu đám Anh Tiên–Song Ngư (Perseus-Pisces Supercluster) | ||
| Siêu đám Khổng Tước–Ấn Đệ An (Pavo-Indus Supercluster) | In 2014, the newly announced Laniakea Supercluster subsumed the Pavo-Indus Supercluster, which became a component of the new supercluster.[2] | |
| Siêu đám Hậu Phát (Coma Supercluster) | Forms most of the CfA Homunculus, the center of the CfA2 Great Wall galaxy filament | |
| Chòm siêu đám Ngọc Phu (Sculptor Superclusters) | SCl 9 | |
| Chòm siêu đám Vũ Tiên (Hercules Superclusters) | SCl 160 | |
| Siêu đám Sư Tử (Leo Supercluster) | SCl 93 | |
| Siêu đám Xà Phu (Ophiuchus Supercluster) |
| 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.[3] |
| Siêu đám Shapley (Shapley Supercluster) |
| The second supercluster found, after the Local Supercluster. |
| Siêu đám thiên hà | Thông tin | Ghi chú |
|---|---|---|
| Siêu đám Song Ngư–Kình Ngư (Pisces-Cetus Supercluster) | ||
| Siêu đám Mục Phu (Boötes Supercluster) | SCl 138 | |
| Siêu đám Thời Chung (Horologium Supercluster) | z=0.063 (700 Mly)Length = 550 Mly | The entire supercluster is referred to as the Horologium-Reticulum Supercluster |
| Siêu đám Bắc Miện (Corona Borealis Supercluster) | z=0.07[4] | |
| Siêu đám Thiên Cáp (Columba Supercluster) | ||
| Siêu đám Bảo Bình (Aquarius Supercluster) | ||
| Siêu đám Bảo Bình B (Aquarius B Supercluster) | ||
| Siêu đám Bảo Bình–Ma Kết (Aquarius-Capricornus Supercluster) | ||
| Siêu đám Bảo Bình–Kình Ngư (Aquarius-Cetus Supercluster) | ||
| Siêu đám Mục Phu A (Boötes A Supercluster) | ||
| Siêu đám Điêu Cụ (Caelum Supercluster) | SCl 59 | |
| Siêu đám Thiên Long (Draco Supercluster) | ||
| Siêu đám Thiên Long–Đại Hùng (Draco-Ursa Major Supercluster) | ||
| Siêu đám Thiên Lô–Ba Giang (Fornax-Eridanus Supercluster) | ||
| Siêu đám Thiên Hạc (Grus Supercluster) | ||
| Siêu đám Sư Tử A (Leo A Supercluster) | ||
| Siêu đám Sư Tử–Lục Phân Nghi (Leo-Sextans Supercluster) | ||
| Siêu đám Sư Tử–Xử Nữ (Leo-Virgo Supercluster) | SCl 107 | |
| Siêu đám Hiển Vi Kính (Microscopium Supercluster) | SCl 174 | |
| Siêu đám Phi Mã–Song Ngư (Pegasus-Pisces Supercluster) | SCl 3 | |
| Siêu đám Anh Tiên–Song Ngư (Perseus-Pisces Supercluster) | SCl 40 | |
| Siêu đám Song Ngư–Bạch Dương (Pisces-Aries Supercluster) | ||
| Siêu đám Đại Hùng (Ursa Major Supercluster) | ||
| Siêu đám Xử Nữ–Hậu Phát (Virgo-Coma Supercluster) | SCl 111 |
| Siêu đám thiên hà | Thông tin | Ghi chú |
|---|---|---|
| Siêu đám Thiên Miêu (Lynx Supercluster) | z=1.27 | Discovered in 1999[5] (as ClG J0848+4453, a name now used to describe the western cluster, with ClG J0849+4452 being the eastern one),[6] 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.[7] Additionally, seven smaller groups of galaxies are associated with the supercluster.[8] |
| SCL @ 1338+27 at z=1.1 | z=1.1 Length=70Mpc | A rich supercluster with several galaxy clusters was discovered around an unusual concentration of 23 QSOs at z=1.1 in 2001. The size of the complex of clusters may indicate a 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 [9][10] |
| SCL @ 1604+43 at z=0.9 | 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 16h 04m 25.7s, +43° 14′ 44.7″[11] |
| SCL @ 0018+16 at z=0.54 in SA26 | 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.[12] |
| MS 0302+17 | z=0.42 Length=6Mpc | This supercluster has at least three member clusters, the eastern cluster CL 0303+1706, southern cluster MS 0302+1659 and northern cluster MS 0302+1717.[13] |
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