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NGC 1559 is a barred spiral galaxy in the constellation Reticulum. It is also a Seyfert galaxy. Although it was originally thought to be a member of the Dorado Group,[2] subsequent observations have shown that it is in fact not a member of any galaxy group or cluster and does not have any nearby companions.[3][4] NGC 1559 has massive spiral arms and strong star formation.[3] It contains a small bar which is oriented nearly east-west and spans 40″.[3] Its bar and disc are the source of very strong radio emissions.[3]
Four supernovae have been observed in NGC 1559. Australian amateur astronomer Robert Evans[5] discovered the first three: SN 1984J (type II, mag. 13.5),[6] SN 1986L (type II, mag. 13.5),[7] and SN 2005df (Type Ia, mag 12.3).[8] SN 2009ib (type IIP, mag. 14.7)[9] was discovered on 6 August 2009.
^ abcdefg"NASA/IPAC Extragalactic Database", Results for NGC 4650A, retrieved 2007-04-03
^Huchra, J. P.; Geller, M. J. (June 15, 1982), "Groups of galaxies. I - Nearby groups", Astrophysical Journal, 257 (Part 1): 423–437, Bibcode:1982ApJ...257..423H, doi:10.1086/160000
^ abcdBeck, R.; Shoutenkov, V.; Ehle, M.; Harnett, J. I.; et al. (August 2002), "Magnetic fields in barred galaxies. I. The atlas", Astronomy and Astrophysics, 391 (1): 83–102, arXiv:astro-ph/0207201, Bibcode:2002A&A...391...83B, doi:10.1051/0004-6361:20020642, S2CID 14749261
^Maia, M. A. G.; da Costa, L. N.; Latham, David W. (April 1989), "A catalog of southern groups of galaxies", Astrophysical Journal Supplement Series, 69: 809–829, Bibcode:1989ApJS...69..809M, doi:10.1086/191328, ISSN 0067-0049
^"Supernova Discoveries by Rev. Robert Evans". revivals.arkangles.com/. Archived from the original on 3 March 2016. Retrieved 11 July 2015.
^Transient Name Server entry for SN 1984J. Retrieved 25 March 2023.
^Transient Name Server entry for SN 1986L. Retrieved 25 March 2023.
^Transient Name Server entry for SN 2005df. Retrieved 25 March 2023.
^Transient Name Server entry for SN 2009ib. Retrieved 25 March 2023.
NGC1559 is a barred spiral galaxy in the constellation Reticulum. It is also a Seyfert galaxy. Although it was originally thought to be a member of the...
PGC 13818, NGC 1249, and PGC 11139. And the six dropped from the 1982 list were: NGC 2082, NGC 1947, NGC 1796, NGC 1688, NGC 1672, and NGC1559. In 2007...
abductors. In 2005, a type Ia supernova was discovered in the spiral galaxy NGC1559, located in the constellation. The dwarf galaxy Reticulum II is enriched...
include SN 2023ixf in Messier 101 (May 2023), SN 2023idj in NGC 4568 (May 2023) and SN 2023gfo in NGC 4995 (April 2023). In most entries, the year when the...
together with the name of the observing project (HUDF, SDSS, 3C, CFHQS, NGC/IC, etc.) This is a list of galaxies that are well known by something other...
SN 2005df was a Type Ia supernova in the barred spiral galaxy NGC1559, which is located in the southern constellation of Reticulum. The event was discovered...
galaxies. List of NGC objects (1–1000) List of NGC objects (1001–2000) List of NGC objects (2001–3000) List of NGC objects (3001–4000) List of NGC objects (4001–5000)...
of Stars (abbreviated NGC) is an astronomical catalogue of deep-sky objects compiled by John Louis Emil Dreyer in 1888. The NGC contains 7,840 objects...
vol 3, p. 1559 Wikimedia Commons has media related to NGC 6822. The Milky Way's Tiny but Tough Galactic Neighbour — ESO Press Release NGC 6822: Barnard's...
NGC 1512 is a barred spiral galaxy approximately 38 million light-years away from Earth in the constellation Horologium. The galaxy displays a double...
Messier 38 or M38, also known as NGC 1912 or Starfish Cluster, is an open cluster of stars in the constellation of Auriga. It was discovered by Giovanni...
The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated in the Milky Way, being south of Orion's Belt in the constellation...
NGC 1761 (also known as GC 980, JH 2710, LH 9) is an open cluster in the Dorado constellation in the Large Magellanic Cloud. It encompasses a group of...
Messier 36 or M36, also known as NGC 1960 or the Pinwheel Cluster, is an open cluster of stars in the somewhat northern Auriga constellation. It was discovered...
Messier 43 or M43, also known as De Mairan's Nebula and NGC 1982, is a star-forming nebula with a prominent H II region in the equatorial constellation...
NGC 1537 is an elliptical galaxy located around 64 million light-years away in the constellation Eridanus. NGC 1537 is south of the celestial equator and...
NGC 1530 is a barred spiral galaxy in the northern constellation of Camelopardalis. It was discovered by German astronomer W. Tempel in 1876. Danish astronomer...
The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common...
NGC 1616 is an intermediate spiral galaxy located around 213 million light-years away in the constellation Caelum. NGC 1616 was discovered on October 24th...
Messier 79 (also known as M79 or NGC 1904) is a globular cluster in the southern constellation Lepus. It was discovered by Pierre Méchain in 1780 and...
NGC 1819 is a lenticular galaxy in the constellation of Orion. It was discovered on December 26, 1885, by American astronomer Lewis A. Swift. This galaxy...
NGC 1569 is a dwarf irregular galaxy in Camelopardalis. The galaxy is relatively nearby and consequently, the Hubble Space Telescope can easily resolve...
Lambda Persei. The same telescope field contains the clusters NGC 1528 and NGC 1545. NGC 1513 was discovered in 1790 by the German-British astronomer William...
NGC 1947 is a peculiar lenticular galaxy in the constellation Dorado. The galaxy lies about 50 million light years away from Earth, which means, given...
NGC 1566, sometimes known as the Spanish Dancer, is an intermediate spiral galaxy in the constellation Dorado, positioned about 3.5° to the south of the...