| NGC 3414 | |
|---|---|
 legacy surveys image of NGC 3414 (bottom) and NGC 3418 (spiral galaxy at the top) | |
| Observation data (J2000 epoch) | |
| Constellation | Leo Minor |
| Right ascension | 10h 51m 16.242s[1] |
| Declination | +27° 58′ 29.88″[1] |
| Redshift | 0.00485[2] |
| Heliocentric radial velocity | 1450 ± 55 km/s[2] |
| Distance | 77 Mly (23.5 Mpc)[3] |
| Apparent magnitude (V) | 11.09[4] |
| Apparent magnitude (B) | 12.06[4] |
| Characteristics | |
| Type | S0pec[3] |
| Other designations | |
| Arp 162, UGC 5959, MCG +05-26-021, PGC 32533[2] | |
NGC 3414 is a lenticular galaxy in the constellation Leo Minor. It was discovered by William Herschel on April 11, 1785.[5] It is the central galaxy of a rich galaxy group.[3] Two galaxies, NGC 3418 and UGC 5958, have similar redshifts and are within 800,000 light-years (250 kiloparsecs) of NGC 3414.[6] It is a member of the NGC 3504 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[7]
It has a peculiar morphology, and is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 162.[2] The outer disc is nearly face-on, and the inner disk has a higher ellipticity and perhaps a central bar.[3] There is a radio source that is powered by a central active galactic nucleus.[6]
References
- ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- ^ a b c d "NGC 3414". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-05-18.
- ^ a b c d Sil'Chenko, O. K.; Proshina, I. S.; Shulga, A. P.; Koposov, S. E. (2012). "Ages and abundances in large-scale stellar discs of nearby S0 galaxies". Monthly Notices of the Royal Astronomical Society. 427 (1): 790–805. arXiv:1209.0606. Bibcode:2012MNRAS.427..790S. doi:10.1111/j.1365-2966.2012.21990.x.
- ^ a b "Search specification: NGC 3414". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-05-18.
- ^ "New General Catalog Objects: NGC 3400 - 3449".
- ^ a b González-Martín, O.; Masegosa, J.; Márquez, I.; Guainazzi, M.; Jiménez-Bailón, E. (2009). "An X-ray view of 82 LINERs with Chandra and XMM-Newton data". Astronomy & Astrophysics. 506 (3): 1107–1121. arXiv:0905.2973. Bibcode:2009A&A...506.1107G. doi:10.1051/0004-6361/200912288. S2CID 119287783.
- ^ "The Leo III Groups". Atlas of the Universe. Archived from the original on July 22, 2012. Retrieved 2010-11-27.
External links
Media related to NGC 3414 at Wikimedia Commons
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This page was last edited on 18 January 2024, at 18:05