Fornax Wall

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The Fornax Wall is a superstructure known as a galaxy filament or galaxy wall. [1] [2] It is a long filament of galaxies with a major axis longer than its minor one. The filament contains not only Dorado Group but also the Fornax cluster of galaxies, which lies at the same distance. It is "parallel" to the Sculptor Wall and "perpendicular" to the Grus Wall. [3]

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<span class="mw-page-title-main">Virgo Supercluster</span> Galactic supercluster containing the Virgo Cluster

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<span class="mw-page-title-main">Great Attractor</span> Region of overdensity of galaxies within the local supercluster

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<span class="mw-page-title-main">Observable universe</span> All of space observable from the Earth at the present

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<span class="mw-page-title-main">Hydra–Centaurus Supercluster</span> Closest neighboring galaxy supercluster

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<span class="mw-page-title-main">Dwarf spheroidal galaxy</span> Low-luminosity galaxy of old stars & little dust

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<span class="mw-page-title-main">NGC 1365</span> Galaxy in the constellation Fornax

NGC 1365, also known as the Fornax Propeller Galaxy or the Great Barred Spiral Galaxy, is a double-barred spiral galaxy about 75 million light-years away in the constellation Fornax. It was discovered on 2 September 1826 by Scottish astronomer James Dunlop.

<span class="mw-page-title-main">NGC 1300</span> Galaxy in the constellation Eridanus

NGC 1300 is a barred spiral galaxy located about 65 million light-years away in the constellation Eridanus. The galaxy is about 110,000 light-years across. It is a member of the Eridanus Cluster, a cluster of 200 galaxies, in a subgroup of 2-4 galaxies in the cluster known as the NGC 1300 Group. It was discovered by John Herschel in 1835.

<span class="mw-page-title-main">NGC 1427</span> Galaxy in the constellation Fornax

NGC 1427 is a low-luminosity elliptical galaxy located approximately 71 million light-years away from Earth. It was discovered by John Frederick William Herschel on November 28, 1837. It is a member of the Fornax Cluster. The galaxy has a stellar mass of 7.9 × 1010M, and a total mass of 9.4 × 1010M. However, the mass of the dark matter halo surrounding the galaxy is around 4.3 × 1012M.

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<span class="mw-page-title-main">NGC 1399</span> Elliptical galaxy in the Fornax Cluster

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<span class="mw-page-title-main">Sculptor Wall</span>

The Sculptor Wall is a superstructure of galaxies relatively near to the Milky Way Galaxy, also known as the Sculptor superclusters.

<span class="mw-page-title-main">Laniakea Supercluster</span> Galaxy supercluster that is home to the Milky Way Galaxy and many more galaxies

The Laniakea Supercluster or the Local Supercluster is the galaxy supercluster that is home to the Milky Way and approximately 100,000 other nearby galaxies.

<span class="mw-page-title-main">Southern Supercluster</span> Closest neighboring galaxy supercluster

The Southern Supercluster is a nearby supercluster located around 19.5 Mpc (63.6 Mly) in the constellations of Cetus, Fornax, Eridanus, Horologium, and Dorado. It was first identified in 1953 by Gérard de Vaucouleurs.

<span class="mw-page-title-main">NGC 1436</span> Galaxy in the constellation Eridanus

NGC 1436 is a barred spiral galaxy with LINER activity approximately 58 million light-years away from Earth in the constellation of Eridanus. NGC 1436 is a flocculent spiral galaxy lying almost face-on to the Earth. It is a member of the Fornax I cluster.

The Grus Wall is a superstructure of galaxies formed in the early universe, named for the Grus constellation in which it is found. It has an average redshift of z=2.38 and lies about 10.8 billion light-years away. The Wall is around 300 million light-years long, comparable in size to the Sloan Great Wall. The Wall is "perpendicular" to the Fornax Wall and Sculptor Wall.

<span class="mw-page-title-main">NGC 1381</span> Galaxy in the constellation Fornax

NGC 1381 is a lenticular galaxy located in the constellation Fornax. It is located at a distance of about 60 million light years from Earth, which, given its apparent dimensions, means that NGC 1381 is about 55,000 light years across. It is a member of the Fornax Cluster. NGC 1381 appears edge-on and features a thin disk with high surface brightness and a boxy bulge. Both the box-shaped bulge and the kinematics of the central area of the galaxy suggest that NGC 1381 has a bar.

<span class="mw-page-title-main">NGC 1387</span> Galaxy in the constellation Fornax

NGC 1387 is a lenticular galaxy in the constellation Fornax, in the Fornax Cluster. It was discovered by William Herschel on December 25, 1835.

The Telescopium−Grus Cloud is a galaxy filament in the constellations of Pavo, Indus, and Telescopium. It was first defined by astronomer Brent Tully in his book The Nearby Galaxies Atlas and its companion book The Nearby Galaxies Catalog.

The Southern Supercluster Strand is a galaxy filament that incompasses the Southern Supercluster and the Telescopium−Grus Cloud.

References

  1. Maurogordato, S. (1995). Maurogordato, S. (ed.). Clustering in the universe: Les Arcs, Savoie, France, March 11 - 18, 1995. Proceedings of the ... Rencontre de Moriond. Gif-sur-Yvette: Ed. Frontières. p. 69. ISBN   978-2-86332-189-8.
  2. Fairall, A. P.; Paverd, W. R.; Ashley, R. P. (1994). "Visualization of Nearby Large-Scale Structures". Astronomical Society of the Pacific . 67. Harvard University: 21. Bibcode:1994ASPC...67...21F.
  3. O'Meara, Stephen James (2013). Southern gems. Deep-sky companions. Cambridge: Cambridge university press. p. 107. ISBN   978-1-107-01501-2 . Retrieved 11 October 2018.