NGC 4183

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NGC 4183
Hubble portrays a dusty spiral galaxy.jpg
Picture of NGC 4183 created from visible and infrared images taken with the Wide Field Channel of the Advanced Camera for Surveys.
Observation data (J2000 epoch)
Constellation Canes Venatici [1]
Right ascension 12h 13m 16.860s [2]
Declination +43° 41′ 53.77″ [2]
Redshift 0.003105 [2]
Heliocentric radial velocity 929 km/s [2]
Distance 55 million light years [1]
Group or cluster Ursa Major Cluster
Characteristics
Type Sc [2]
Size80,000 ly (diameter)
Apparent size  (V)6.39 x 0.39
Other designations
MCG+07-25-051, UZC J121317.0+434153, [CHM2007] LDC 867 J121316.86+4341537,

FGC 1386, 2MFGC 9620, Z 215-53, LEDA 38988, RFGC 2222, Z 1210.7+4358,

2MASX J12131686+4341537, UGC 7222, [CHM2007] HDC 706 J121316.86+4341537

NGC 4183 is a spiral galaxy with a faint core and an open spiral structure located about 55 million light-years from the Sun. Spanning about eighty thousand light-years, it appears in the constellation of Canes Venatici. NGC 4183 was observed for the first time by British astronomer William Herschel on 14 January 1788.

NGC 4183 is a member of the NGC 4111 Group, [3] [4] which is part of the Ursa Major Cloud and is the second largest group in the cloud after the NGC 3992 Group. [5] [6] [7]

One supernova has been observed in NGC 4183: SN 1968U (type unknown, mag. 14.5) was discovered by Justus R. Dunlap on 29 October 1968. [8] [9]

References

  1. 1 2 "Hubble portrays a dusty spiral galaxy". ESA/Hubble Picture of the Week. Retrieved 27 September 2012.
  2. 1 2 3 4 5 "Search Results for NGC 4183". Astronomical Database. SIMBAD . Retrieved 27 September 2012.
  3. ↑ Makarov, Dmitry; Karachentsev, Igor (2011-04-21). "Galaxy groups and clouds in the local (z∼ 0.01) Universe: Galaxy groups in the local Universe". Monthly Notices of the Royal Astronomical Society. 412 (4): 2498–2520. arXiv: 1011.6277 . doi: 10.1111/j.1365-2966.2010.18071.x .
  4. ↑ Kourkchi, Ehsan; Tully, R. Brent (2017-07-01). "Galaxy Groups Within 3500 km s −1". The Astrophysical Journal. 843 (1): 16. arXiv: 1705.08068 . doi: 10.3847/1538-4357/aa76db . ISSN   0004-637X.
  5. ↑ Karachentsev, I. D.; Nasonova, O. G.; Courtois, H. M. (2013-03-01). "Anatomy of Ursa Majoris". Monthly Notices of the Royal Astronomical Society. 429 (3): 2264–2273. arXiv: 1211.5975 . doi: 10.1093/mnras/sts494 . ISSN   1365-2966.
  6. ↑ Pak, Mina; Rey, Soo-Chang; Lisker, Thorsten; Lee, Youngdae; Kim, Suk; Sung, Eon-Chang; Jerjen, Helmut; Chung, Jiwon (2014-09-29). "The properties of early-type galaxies in the Ursa Major cluster". Monthly Notices of the Royal Astronomical Society. 445 (1): 630–647. arXiv: 1409.3070 . doi: 10.1093/mnras/stu1722 . ISSN   0035-8711.
  7. ↑ Ai, Mei; Zhu, Ming; Yu, Nai-ping; Xu, Jin-long; Liu, Xiao-lan; Jing, Yingjie; Jiao, Qian; Liu, Yao; Zhang, Chuan-peng; Wang, Jie; Jiang, Peng (2025-04-01). "Formation of the Dark Matter–Deficient S0 Galaxy NGC 4111 under the Tidal Interactions". The Astrophysical Journal Letters. 982 (2): L52. arXiv: 2503.05171 . Bibcode:2025ApJ...982L..52A. doi: 10.3847/2041-8213/adbeee . ISSN   2041-8205.
  8. ↑ Gingerich, Owen (31 October 1968). "Circular No. 2109". Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory. Retrieved 2 December 2024.
  9. ↑ "SN 1968U". Transient Name Server. IAU . Retrieved 2 December 2024.
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