PGC 4976, GC 280, 2MASS J01221356+0525012, Z 411.36, MGC +01-04-038
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NGC 492, also occasionally referred to as PGC 4976 or GC 280, is a barred spiral galaxy in the constellation Pisces.[1] It is located approximately 590 million light-years from Earth and was discovered on December 6, 1850 by Irish engineer Bindon Blood Stoney.[2] Although John Dreyer, creator of the New General Catalogue, credits the discovery to astronomer William Parsons, 3rd Earl of Rosse, he notes that many of his claimed discoveries were made by one of his assistants. In the case of NGC 492, the discovery was made by Bindon Stoney,[3] who discovered it along with NGC 486, NGC 490 and NGC 500 during his observation of NGC 488 using Lord Rosse's 72" telescope. [4]
The object was initially described by Stoney as "extremely faint, small, round, 25" diameter, low surface brightness, no concentration". The position noted was "on line with a mag 12 star 3.7' NW and a faint pair of mag 14-14.5 stars 2' NW".[5]
^"Revised NGC Data for NGC 492". spider.seds.org. Retrieved 2017-10-05.
^"Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-05.
^"New General Catalog Objects: NGC 450 - 499". cseligman.com. Retrieved 2017-10-16.
NGC492, also occasionally referred to as PGC 4976 or GC 280, is a barred spiral galaxy in the constellation Pisces. It is located approximately 590 million...
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case of NGC 490, the discovery was made by Bindon Stoney, who discovered it along with NGC 486, NGC492 and NGC 500 during his observation of NGC 488. The...
case of NGC 486, the discovery was made by Bindon Stoney, who discovered it along with NGC 490, NGC492 and NGC 500 during his observation of NGC 488 using...
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"Kinematics of the Nuclear Ionized Gas in the Radio Galaxy M84 (NGC 4374)". Astrophysical Journal. 492 (1): 111–114. arXiv:astro-ph/9710264. Bibcode:1998ApJ.....
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Na–O relation in the bulge globular cluster NGC 6553", Monthly Notices of the Royal Astronomical Society, 492 (3): 3742–3752, arXiv:1912.03742, doi:10.1093/mnras/stz3586...
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"Evolutionary status and age spread in the young LMC cluster NGC 1850A". Astronomy and Astrophysics. 330: 492–504. Bibcode:1998A&A...330..492C. Fischer, Philippe;...
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"Kinematics of the Nuclear Ionized Gas in the Radio Galaxy M84 (NGC 4374)". Astrophysical Journal. 492 (1): 111–114. arXiv:astro-ph/9710264. Bibcode:1998ApJ.....
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bright elliptical galaxy NGC 3613 and its globular cluster system". Monthly Notices of the Royal Astronomical Society. 492 (3): 4313–4324. arXiv:2005...
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originally named the Andromeda Nebula and is cataloged as Messier 31, M31, and NGC 224. Andromeda has a D25 isophotal diameter of about 46.56 kiloparsecs (152...