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// Workers AI · dad joke modeWhat did NGC 3414 say to its friend? You're a galaxy ahead.

Coordinates: Sky map 10h 51m 16.242s, +27° 58′ 29.88″
From Wikipedia, the free encyclopedia
(Redirected from Arp 162)
NGC 3414
NGC 3414
legacy surveys image of NGC 3414 (bottom) and NGC 3418 (spiral galaxy at the top)
Observation data (J2000 epoch)
ConstellationLeo Minor
Right ascension10h 51m 16.242s[1]
Declination+27° 58′ 29.88″[1]
Redshift0.00485[2]
Heliocentric radial velocity1450 ± 55 km/s[2]
Distance77 Mly (23.5 Mpc)[3]
Apparent magnitude (V)11.09[4]
Apparent magnitude (B)12.06[4]
Characteristics
TypeS0pec[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]

LDC 763 Galaxy group

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NGC 3414 is the central member of the LDC 763 galaxy group, which also includes the neighboring galaxies NGC 3418 and UGC 5958.[8]

See also

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2MASS image of NGC 3414

References

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  1. 1 2 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.
  2. 1 2 3 4 "NGC 3414". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-05-18.
  3. 1 2 3 4 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.
  4. 1 2 "Search specification: NGC 3414". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-05-18.
  5. ↑ "New General Catalog Objects: NGC 3400 - 3449".
  6. 1 2 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.
  7. ↑ "The Leo III Groups". Atlas of the Universe. Retrieved 2010-11-27.{{cite web}}: CS1 maint: deprecated archival service (link)
  8. ↑ Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen; Jarrett, Tom; Macri, Lucas M. (2007-02-20). "Three-Dimensional Groups of Galaxies with the Two Micron All Sky Survey Extended Source Catalog". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610797. Bibcode:2007ApJ...655..790C. doi:10.1086/510115.
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  • Wikimedia Commons logo Media related to NGC 3414 at Wikimedia Commons


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