|
Sculptor Group
The Sculptor Group is a loose group of galaxies visible near the south galactic pole. The group is one of the closest groups of galaxies to the Local Group; the distance to the center of the group from the Milky Way is approximately . The Sculptor Galaxy (NGC 253) and a few other galaxies form a gravitationally-bound core in the center of this group. A few other galaxies at the periphery may be associated with the group but may not be gravitationally bound. Because most of the galaxies in this group are actually weakly gravitationally bound, the group may also be described as a filament. It is considered to be at an early stage of evolution in which galaxies are still falling into the group along filamentary structures. Members The table below lists galaxies that have been identified as associated with the Sculptor Galaxy (and hence associated with the group) by I. D. Karachentsev and collaborators. The object names used in the above table differ from the names used by Kar ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Ngc253 2mass Barred Spiral
NGC commonly refers to: * New General Catalogue of Nebulae and Clusters of Stars, a catalogue of deep sky objects in astronomy NGC may also refer to: Companies * NGC Corporation, name of US electric company Dynegy, Inc. from 1995 to 1998 * National Gas Company of Trinidad and Tobago, state-owned natural gas company in Trinidad and Tobago * National Grid plc, a former name of National Grid Electricity Transmission plc, the operator of the British electricity transmission system * Northrop Grumman Corporation, aerospace and defense conglomerate formed from the merger of Northrop Corporation and Grumman Corporation in 1994 * Numismatic Guaranty Corporation, coin certification company in the United States Other uses * National Gallery of Canada, art gallery founded in 1880 in Ottawa, Canada * National Geographic, documentary and reality television channel established in the United States in 2001 formerly called National Geographic Channel * Native Girls Code, US non-profit organi ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Redshift
In physics, a redshift is an increase in the wavelength, and corresponding decrease in the frequency and photon energy, of electromagnetic radiation (such as light). The opposite change, a decrease in wavelength and simultaneous increase in frequency and energy, is known as a negative redshift, or blueshift. The terms derive from the colours red and blue which form the extremes of the visible light spectrum. In astronomy and cosmology, the three main causes of electromagnetic redshift are # The radiation travels between objects which are moving apart (" relativistic" redshift, an example of the relativistic Doppler effect) #The radiation travels towards an object in a weaker gravitational potential, i.e. towards an object in less strongly curved (flatter) spacetime (gravitational redshift) #The radiation travels through expanding space (cosmological redshift). The observation that all sufficiently distant light sources show redshift corresponding to their distance from Earth ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
UGCA 15
The Uppsala General Catalogue of Galaxies (UGC) is a catalogue of 12,921 galaxies visible from the northern hemisphere. It was first published in 1973. The catalogue includes essentially all galaxies north of declination -02°30' and to a limiting diameter of 1.0 arcminute or to a limiting apparent magnitude of 14.5. The primary source of data is the blue prints of the Palomar Observatory Sky Survey (POSS). It also includes galaxies smaller than 1.0 arcminute in diameter but brighter than 14.5 magnitude from the Catalogue of Galaxies and of Clusters of Galaxies (CGCG). The catalogue contains descriptions of the galaxies and their surrounding areas, plus conventional system classifications and position angles for flattened galaxies. Galaxy diameters are included and the classifications and descriptions are given in such a way as to provide as accurate an account as possible of the appearance of the galaxies on the prints. The accuracy of coordinates is only what is necessary for ide ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Sculptor Dwarf Irregular Galaxy
The Sculptor Dwarf Irregular Galaxy (SDIG) is an irregular galaxy in the constellation Sculptor. It is a member of the NGC 7793 subgroup of the Sculptor Group. The galaxy was discovered in 1976. __NOTOC__ Nearby galaxies and galaxy group information The Sculptor Dwarf Irregular Galaxy and the dwarf galaxy UGCA 442 are both companions of the spiral galaxy NGC 7793. These galaxies all lie within the Sculptor Group, a weakly bound, filament-like group of galaxies located near the Local Group. See also * Sculptor Dwarf Galaxy The Sculptor Dwarf Galaxy (also known as Sculptor Dwarf Elliptical Galaxy or the Sculptor Dwarf Spheroidal Galaxy, and formerly as the Sculptor System) is a dwarf spheroidal galaxy that is a satellite of the Milky Way. The galaxy lies within the ... – a dwarf spheroidal or elliptical galaxy, also in Sculptor, but significantly closer; a satellite of the Milky Way. References External links * Dwarf irregular galaxies Sculptor Group Sculptor (cons ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
PGC 6430
PGC may refer to: *Pennsylvania Game Commission *Persian Gulf Cup, Iran's highest association football league *PGC (gene) *PGC 1000714, a ring galaxy *PGC-1α, a protein which is the master regulator of mitochondrial biogenesis *Playwrights Guild of Canada * Postgraduate Certificate, usually written as PgC *Presbyterian Girls' College in Warwick, Australia, now part of Scots PGC College *Primordial germ cell *Prince George's County, Maryland *Principal Galaxies Catalogue *Principle of Generic Consistency, see Alan Gewirth *Professional Graphics Controller * Program chain, which defines the order in which cells, tiles (video, menus, etc.) are played back on a DVD *Psychiatric Genomics Consortium, founded 2007 as the Psychiatric Genome Wide Association Consortium *Punjab Group of Colleges, Pakistan *The University of Pennsylvania Glee Club Founded in 1862, the University of Pennsylvania Glee Club (Penn Glee Club) is one of the oldest continually running glee clubs in the United State ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
PGC 2933
PGC or LEDA 2933 is a faint dwarf irregular galaxy in the Sculptor Group. It can be seen in the southern constellation Phoenix. According to measurements, the galaxy is located 11.15 million light-years away. Because it is situated in the Sculptor Group, it is one of the closest galaxies to the Milky Way The Milky Way is the galaxy that includes our Solar System, with the name describing the galaxy's appearance from Earth: a hazy band of light seen in the night sky formed from stars that cannot be individually distinguished by the naked eye .... It is obscured by a few brighter stars and galaxies (the brightest of them on the right side of the photo is 1425 light-years away from the Solar System). The galaxy has a 2000 light-year diameter. References {{reflist, refs= {{Cite web , title=ESO 540-32 , url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=PGC+2933&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id , access-date=2022-08-28 , website=simbad.u-strasbg.f ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
ESO 540-030
ESO 540-030 is a faint dwarf galaxy in the Sculptor Group. It has the appearance of a massive scattering of dim stars. The galaxy is located slightly more than 11 million light-years from Earth. It is difficult to observe due to galaxies situated behind ESO 540-030, and five bright stars between the galaxy and the Solar System The Solar SystemCapitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Solar S .... The brightest of them is located around 1500 light-years away from us. References {{DEFAULTSORT:ESO 540-030 Sculptor Group Dwarf galaxies Sculptor (constellation) 540-030 002881 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
NGC 7793
NGC 7793 is a flocculent spiral galaxy in the southern constellation of Sculptor. It was discovered in 1826 by Scottish astronomer James Dunlop. The galaxy is located at a distance of million light years and is receding with a heliocentric radial velocity of . NGC 7793 is one of the five brightest galaxies within the Sculptor Group. The morphological class of NGC 7793 is SA(s)d, indicating it is unbarred spiral galaxy (SA) with no inner ring structure (s) and the arms are loosely wound and disorganized (d). It is flocculent in appearance with a very small bulge and a star cluster at the nucleus. The galactic disk is inclined at an angle of 53.7° to the line of sight from the Earth. The visible profile is elliptical in form with an angular size of and a major axis aligned along a position angle of 99.3°. There are two nearby dwarf galaxy companions. On March 25, 2008, a type II-P supernova designated SN 2008bk was discovered in NGC 7793. At apparent magnitude 12.5, it be ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
NGC 625
NGC 625 is a dwarf barred spiral galaxy about 12.7 Mly away in the constellation Phoenix. NGC 625 is a member of the Sculptor Group The Sculptor Group is a loose group of galaxies visible near the south galactic pole. The group is one of the closest groups of galaxies to the Local Group; the distance to the center of the group from the Milky Way is approximately . The Sculp .... References External links * * NGC 0625 NGC 0625 NGC 0625 NGC 0625 0625 05896 {{Spiral-galaxy-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
NGC 247
NGC 247 (also known as Caldwell 62 and commonly known as the Claw Galaxy) is an intermediate spiral galaxy (although it is sometimes classified as a dwarf spiral galaxy) about 11.1 Mly away in the constellation Cetus. This distance was confirmed in late February 2011. Previous measurements showed that the galaxy was about 12.2 Mly away, but this was proved to be wrong. NGC 247 is a member of the Sculptor Group, and is 70 000 light years in diameter. NGC 247 has an unusually large void on one side of its spiral disk. This void contains some older, redder stars but no younger, bluer stars. Nearby galaxies and galaxy group information NGC 247 is one of several galaxies that is gravitationally bound to the Sculptor Galaxy (NGC 253). These galaxies form a small core in the center of the Sculptor Group, which is one of the nearest groups of galaxies to the Milky Way The Milky Way is the galaxy that includes our Solar System, with the name describing the galaxy's appearan ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
NGC 59
NGC 59 is a lenticular galaxy in the constellation Cetus. It is a probable member of the Sculptor Group The Sculptor Group is a loose group of galaxies visible near the south galactic pole. The group is one of the closest groups of galaxies to the Local Group; the distance to the center of the group from the Milky Way is approximately . The Sculp .... It is approximately 17 million light-years away. References External linksSEDS* * {{DEFAULTSORT:NGC 59 Lenticular galaxies 0059 01034 -04-01-026 539-G4 18851110 Cetus (constellation) ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
