NGC 1260

NGC 1260
NGC 1260
	NGC 1260 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation	Perseus
Right ascension	03h 17m 27.2s
Declination	+41° 24′ 19″
Redshift	0.01919
Helio radial velocity	5753 ± 14 km/s
Distance	250 ± 1.6 Mly; (76.7 ± 0.5 Mpc)
Apparent magnitude (V)	14.3
Characteristics
Type	S0/a
Apparent size (V)	1′.1 × 0′.5
Other designations
	UGC 02634, PGC 012219, MCG +07-07-047

NGC 1260 is a spiral or lenticular galaxy^[3] in the constellation Perseus.^[4] It was discovered by astronomer Guillaume Bigourdan on October 19, 1884.^[5] NGC 1260 is a member of the Perseus Cluster^[6]^[3] and forms a tight pair with the galaxy .^[3] In 2006, it was home to the second brightest supernova in the observable universe, supernova SN 2006gy.

Supernova 2006gy imaged by the Swift spacecraft

References[]

^ ^a ^b ^c ^d ^e ^f ^g ^h "NASA/IPAC Extragalactic Database". Results for NGC 1260. Retrieved 7 May 2007.
^ "Distance Results for NGC 1260". NASA/IPAC Extragalactic Database. Retrieved 4 May 2010.
^ ^a ^b ^c Hakobyan, A. A.; Petrosian, A. R.; McLean, B.; Kunth, D.; Allen, R. J.; Turatto, M.; Barbon, R. (24 June 2008). "Early-type galaxies with core collapse supernovae". Astronomy & Astrophysics. 488 (2): 523–531. arXiv:0806.4269. Bibcode:2008A&A...488..523H. doi:10.1051/0004-6361:200809817. ISSN 0004-6361. S2CID 17273642.
^ "Revised NGC Data for NGC 1260". spider.seds.org. Retrieved 17 June 2018.
^ "New General Catalog Objects: NGC 1250 - 1299". cseligman.com. Retrieved 17 June 2018.
^ Brunzendorf, J.; Meusinger, H. (1 October 1999). "The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types". Astronomy and Astrophysics Supplement Series. 139 (1): 141–161. Bibcode:1999A&AS..139..141B. doi:10.1051/aas:1999111. ISSN 0365-0138.