Arp 256 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 00h 18m 50.898s [1] |
Declination | −10° 22′ 36.49″ [1] |
Redshift | 0.027 [1] |
Helio radial velocity | 7985 km/s [1] |
Distance | 380 Mly (115 Mpc) [2] |
Apparent magnitude (V) | S: 14.33 [1] N: 13.60 [1] |
Apparent magnitude (B) | S: 14.81 [1] N: 13 [1] |
Characteristics | |
Type | S: SB(s)b pec? [2] N: SB(s)c pec [2] |
Apparent size (V) | S: 1.1′ × 0.6′ [3] N: 1.1′ × 0.8′ [4] |
Notable features | Interacting galaxies |
Other designations | |
Arp 256S: MCG-02-01-051, PGC 1224 [1] Arp 256N: MCG-02-01-052, PGC 1221 [4] |
Arp 256 is a pair of interacting spiral galaxies located in the constellation of Cetus. Arp 256 (also Arp 256S) refers to the southern galaxy; [1] the northern galaxy is Arp 256N. [4]
The NASA/IPAC Extragalactic Database (NED) is an online astronomical database for astronomers that collates and cross-correlates astronomical information on extragalactic objects. NED was created in the late 1980s by two Pasadena astronomers, George Helou and Barry F. Madore. NED is funded by NASA and is operated by the Infrared Processing and Analysis Center (IPAC) on the campus of the California Institute of Technology, under contract with NASA.
The Atlas of Peculiar Galaxies is a catalog of peculiar galaxies produced by Halton Arp in 1966. A total of 338 galaxies are presented in the atlas, which was originally published in 1966 by the California Institute of Technology. The primary goal of the catalog was to present photographs of examples of the different kinds of peculiar structures found among galaxies.
Arp 87 is a pair of interacting galaxies, NGC 3808A and NGC 3808B. They are situated in the Leo constellation. NGC 3808A, the brighter, is a peculiar spiral galaxy, while NGC 3808B is an irregular galaxy.
NGC 559 is an open cluster and Caldwell object in the constellation Cassiopeia. It shines at magnitude +9.5. Its celestial coordinates are RA 01h 29.5m, dec +63° 18′. It is located near the open cluster NGC 637, and the bright magnitude +2.2 irregular variable star Gamma Cassiopeiae. The cluster is 7 arcmins across.
NGC 9 is a spiral galaxy about 140 million light-years away in the Pegasus constellation. It was discovered on 27 September 1865 by Otto Wilhelm von Struve.
NGC 3561, also known as Arp 105, is a pair of interacting galaxies NGC 3561A and NGC 3561B within the galaxy cluster Abell 1185 in Ursa Major. Its common name is "the Guitar" and contains a small tidal dwarf galaxy known as Ambartsumian's Knot that is believed to be the remnant of the extensive tidal tail pulled out of one of the galaxies.
AM 1316-241 is a pair of overlapping galaxies in the constellation Hydra. It is notable for having recently been discovered to have revealed visible dust by the back light from the more distant galaxy of the two.
NGC 6248 is a barred spiral galaxy in the constellation Draco. It was discovered on August 11, 1885 by the American astronomer Lewis A. Swift. The galaxy is located approximately 52 million light years away from earth with an approximate diameter of 47,000 light-years.
KKR 03 is a dwarf irregular galaxy located 6.4 million light-years away from Earth. It has an absolute magnitude of −10.85 and lies on the inner edge of the M94 Group.
NGC 150 is a barred spiral galaxy in the constellation Sculptor. It is about 70 million light years away from the Solar System, and it has a diameter of about 55,000 light years. It was discovered on 20 November 1886, by Lewis A. Swift. The Type II supernova SN 1990K was detected in NGC 150, and was reported to be similar to SN 1987A.
NGC 156 is a double star located in the Cetus constellation. It was discovered on 1882 by Ernst Wilhelm Leberecht Tempel.
NGC 7028 is the designation of a celestial object in the constellation of Delphinus. The object was supposedly discovered by the German astronomer Albert Marth on 17 September 1863. However, its identification is uncertain, and the object is considered lost. No galaxies or nebulous objects are at the coordinates that he gave.
NGC 5575 is a lenticular galaxy in the constellation Virgo. The object was discovered on May 8, 1864 by the German astronomer Albert Marth.
NGC 5030 is a barred spiral galaxy in the constellation Virgo. The object was discovered on 17 March 1881 by the American astronomer Edward Singleton Holden.
NGC 4918 is a spiral galaxy in the constellation Virgo. The object was discovered in 1886 by the American astronomer Francis Preserved Leavenworth.
NGC 3545B is an elliptical galaxy in the constellation Ursa Major. The object is close to NGC 3545.
NGC 3402, also known as NGC 3411, is an elliptical galaxy in the constellation Hydra. The object was discovered on March 25, 1786 by German-British astronomer William Herschel. NGC 3402 is the largest galaxy in the eponymous NGC 3402 cluster.
NGC 7041B is a spiral or lenticular galaxy in the constellation Indus. The object was discovered on 7 July 1834 by the British astronomer John Herschel.
NGC 191A is a lenticular galaxy in the constellation Cetus.
NGC 528 is a lenticular galaxy located in the constellation Andromeda. It is located an estimated 70 million parsecs from the Milky Way. The object was discovered on 22 August 1865 by the German-Danish astronomer Heinrich Ludwig d'Arrest.