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Galaxy Filament
In cosmology, galaxy filaments (subtypes: supercluster complexes, galaxy walls, and galaxy sheets) Boris V. Komberg, Andrey V. Kravtsov, Vladimir N. Lukash; "The search and investigation of the Large Groups of Quasars" ; ;R.G. Clowes; "Large Quasar Groups - A Short Review"; ''The New Era of Wide Field Astronomy'', ASP Conference Series, vol. 232.; 2001; Astronomical Society of the Pacific; ; are the largest known structures in the universe, consisting of walls of gravitationally bound galaxy superclusters. These massive, thread-like formations can reach 80 megaparsecs ''h''−1 (or of the order of 160 to 260 million light-years) and form the boundaries between large voids. Formation In the standard model of the evolution of the universe, galactic filaments form along and follow web-like strings of dark matter—also referred to as the galactic web or cosmic web. It is thought that this dark matter dictates the structure of the Universe on the grandest of scales. Dark matter g ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Galaxy Fimament
A galaxy is a system of stars, stellar remnants, interstellar gas, dust, dark matter, bound together by gravity. The word is derived from the Greek ' (), literally 'milky', a reference to the Milky Way galaxy that contains the Solar System. Galaxies, averaging an estimated 100 million stars, range in size from dwarfs with less than a hundred million stars, to the largest galaxies known – supergiants with one hundred trillion stars, each orbiting its galaxy's center of mass. Most of the mass in a typical galaxy is in the form of dark matter, with only a few percent of that mass visible in the form of stars and nebulae. Supermassive black holes are a common feature at the centres of galaxies. Galaxies are categorized according to their visual morphology as elliptical, spiral, or irregular. Many are thought to have supermassive black holes at their centers. The Milky Way's central black hole, known as Sagittarius A*, has a mass four million times greater than the Sun ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Huge-LQG
The Huge Large Quasar Group, (Huge-LQG, also called U1.27) is a possible structure or pseudo-structure of 73 quasars, referred to as a large quasar group, that measures about 4 billion light-years across. At its discovery, it was identified as the largest and the most massive known structure in the observable universe, though it has been superseded by the Hercules–Corona Borealis Great Wall at 10 billion light-years. There are also issues about its structure (see ''Dispute'' section below). Discovery Roger G. Clowes, together with colleagues from the University of Central Lancashire in Preston, United Kingdom, had reported on January 11, 2013 a grouping of quasars within the vicinity of the constellation Leo. They used data from the DR7QSO catalogue of the comprehensive Sloan Digital Sky Survey, a major multi-imaging and spectroscopic redshift survey of the sky. They reported that the grouping was, as they announced, the largest known structure in the observable universe. ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
ClG J2143-4423
A galaxy cluster, or a cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity, with typical masses ranging from 1014 to 1015 solar masses. They are the second-largest known gravitationally bound structures in the universe after galaxy filaments and were believed to be the largest known structures in the universe until the 1980s, when superclusters were discovered. One of the key features of clusters is the intracluster medium (ICM). The ICM consists of heated gas between the galaxies and has a peak temperature between 2–15 keV that is dependent on the total mass of the cluster. Galaxy clusters should not be confused with ''galactic clusters'' (also known as open clusters), which are star clusters ''within'' galaxies, or with globular clusters, which typically orbit galaxies. Small aggregates of galaxies are referred to as galaxy groups rather than clusters of galaxies. The galaxy groups and ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lynx–Ursa Major Supercluster
Lynx–Ursa Major Supercluster is a supercluster in the Lynx–Ursa Major Region. It was discovered by Giovanelli and Haynes in 1982. The supercluster is connected to Lynx–Ursa Major Filament. References Galaxy superclusters {{supercluster-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lynx–Ursa Major Filament
Lynx–Ursa Major Filament (LUM Filament) is a galaxy filament. The filament is connected to and separate from the Lynx–Ursa Major Supercluster Lynx–Ursa Major Supercluster is a supercluster in the Lynx–Ursa Major Region. It was discovered by Giovanelli and Haynes in 1982. The supercluster is connected to Lynx–Ursa Major Filament. References Galaxy superclusters {{superclus .... References Galaxy filaments Large-scale structure of the cosmos {{physical-cosmology-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
CfA Homunculus
CFA may refer to: * CFA franc, a currency used by fourteen African countries * Chartered Financial Analyst, an international investment professional designation * Chick-fil-A, US fast food chain Agreements * Canadian Football Act * Ceasefire agreement * Compact of Free Association, agreement between US, Micronesia, Marshall Islands, and Palau * Conditional fee agreement, a legal agreement also known as "no win no fee" Medicine * Common femoral artery * Complete Freund's adjuvant, an immunopotentiator composed of inactivated and dried mycobacteria * Cryptogenic fibrosing alveolitis, an archaic term for idiopathic pulmonary fibrosis Organizations * California Faculty Association, the union representing employees at California State University system * Call For Action, telephone help-lines of radio stations in the United States * Campaign for Accountability, a non-profit organization in the United States * Consumer Federation of America, consumer group * Consumers' Federati ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Ursa Major Filament
Ursa Major Filament is a galaxy filament. The filament is connected to the CfA Homunculus, a portion of the filament forms a portion of the "leg" of the Homunculus.''The Astrophysical Journal Supplement Series'', Volume 121, Issue 2, pp. 445-472. "Photometric Properties of Kiso Ultraviolet-Excess Galaxies in the Lynx-Ursa Major Region" ''04/1999'' See also * Abell catalogue The Abell catalog of rich clusters of galaxies is an all-sky catalog of 4,073 rich galaxy clusters of nominal redshift ''z'' ≤ 0.2. This catalog supplements a revision of George O. Abell's original "Northern Survey" of 1958, wh ... * Large-scale structure of the universe * Supercluster References Galaxy filaments Large-scale structure of the cosmos {{physical-cosmology-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Perseus–Pisces Supercluster
The Perseus–Pisces Supercluster (SCl 40) is one of the largest known structures in the universe. Even at a distance of 250 million light-years, this chain of galaxy clusters extends more than 40° across the northern winter sky. The Perseus- Pisces Supercluster is one of two dominant concentrations of galaxies (the other being the Local supercluster) in the nearby universe (within 300 million light years). This supercluster also borders a prominent void, the Taurus Void, and is part of the Perseus–Pegasus Filament which stretches for roughly a billion light years.'Astrophysical Journal', Part 1 (), vol. 299, Dec. 1, 1985, p. 5-14. "A possible 300 megaparsec filament of clusters of galaxies in Perseus-Pegasus" ''12/1985'' Clusters The main clusters of the Perseus–Pisces Supercluster are Abell 262, Abell 347, and Abell 426. See also * Abell catalogue * Large-scale structure of the universe * List of Abell clusters The Abell catalogue is a catalogue of approximate ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Perseus–Pegasus Filament
The Perseus–Pegasus Filament is a galaxy filament containing the Perseus–Pisces Supercluster and stretching for roughly a billion light-years (or over 300/h Mpc). Currently, it is considered to be one of the largest known structures in the universe.The reference cited claims the Perseus-Pisces Filament as the largest known structure in the universe. However, various reports cite the Hercules–Corona Borealis Great Wall as the largest at across. This filament is adjacent to the Pisces–Cetus Supercluster Complex. Discovery The Perseus–Pegasus Filament was discovered by David Batuski and Jack Burns of New Mexico State University in 1985. It is likely that Clyde W. Tombaugh, of the Lowell Observatory, discovered its existence in 1936 while conducting his search for trans-Saturnian planets. He reported it as the Great Perseus-Andromeda stratum of Extra-Galactic Nebulae. Earlier still, parts of this clustering had been reported by .Nature, volume 130, issue 3273, pp. 132 (1 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Coma Supercluster
The Coma Supercluster (SCl 117) is a nearby supercluster of galaxies comprising the Coma Cluster (Abell 1656) and the Leo Cluster (Abell 1367). Located 300 million light-years from Earth, it is in the center of the Great Wall and a part of the Coma Filament. The Coma Supercluster is the nearest massive cluster of galaxies to our own Virgo Supercluster. It is roughly spherical, about 20 million light-years in diameter and contains more than 3,000 galaxies. It is located in the constellation Coma Berenices. Being one of the first superclusters to be discovered, the Coma Supercluster helped astronomers understand the large scale structure of the universe. See also * Abell catalogue * Large-scale structure of the universe * List of Abell clusters The Abell catalogue is a catalogue of approximately 4,000 galaxy clusters with at least 30 members, almost complete to a redshift of ''z'' = 0.2. It was originally compiled by the American astronomer George O. Abell in 1958 using plates ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
