Jump to content

NGC 2004

From Wikipedia, the free encyclopedia
The printable version is no longer supported and may have rendering errors. Please update your browser bookmarks and please use the default browser print function instead.
NGC 2004
Hubble Space Telescope image of NGC 2004
Observation data (J2000 epoch)
Right ascension05h 30m 41.340s[1]
Declination−67° 17′ 21.83″[1]
Distance163.1 ± 0.3 ly (50 ± 0.1 pc)[2]
Apparent magnitude (V)9.6[3]
Apparent dimensions (V)3.0' × 2.8'[4]
Physical characteristics
Mass~2.3×104[5] M
Estimated age20 Ma[5]
Other designationsNGC 2004, ESO 86-SC4[3]
Associations
ConstellationDorado
See also: Open cluster, List of open clusters

NGC 2004 (also known as ESO 86-SC4) is an open cluster of stars in the southern constellation of Dorado. It was discovered by Scottish astronomer James Dunlop on September 24, 1826.[6] This is a young, massive cluster with an age of about 20 million years and 23,000 times the mass of the Sun.[5] It has a core radius of 2.85 ± 0.46 pc (9.3 ± 1.5 ly).[7] NGC 2004 is a member of the Large Magellanic Cloud,[4] which is a satellite galaxy of the Milky Way.

References

  1. ^ a b Werchan, Felicia; Zaritsky, Dennis (2011). "The Star Clusters of the Large Magellanic Cloud: Structural Parameters". The Astronomical Journal. 142 (2): 48. arXiv:1105.1769. Bibcode:2011AJ....142...48W. doi:10.1088/0004-6256/142/2/48. S2CID 118331608.
  2. ^ Beasor, Emma R.; et al. (June 2019). "Discrepancies in the ages of young star clusters; evidence for mergers?". Monthly Notices of the Royal Astronomical Society. 486 (1): 266–273. arXiv:1903.05106. Bibcode:2019MNRAS.486..266B. doi:10.1093/mnras/stz732.
  3. ^ a b "NGC 2004". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 28 May 2019.
  4. ^ a b Bica, E.; et al. (September 2008). "A general catalogue of extended objects in the Magellanic System". Monthly Notices of the Royal Astronomical Society. 389 (2): 678–690. arXiv:0806.3049. Bibcode:2008MNRAS.389..678B. doi:10.1111/j.1365-2966.2008.13612.x. S2CID 1867090.
  5. ^ a b c Niederhofer, F.; et al. (March 2015). "No evidence for significant age spreads in young massive LMC clusters". Astronomy & Astrophysics. 575: 18. arXiv:1501.02275. Bibcode:2015A&A...575A..62N. doi:10.1051/0004-6361/201424455. S2CID 54754949. A62.
  6. ^ Seligman, Courtney. "New General Catalog Objects: NGC 2000 - 2049". New General Catalog Objects: NGC 2000 - 2049. Retrieved 28 May 2019.
  7. ^ Nikolov, Grigor; Markov, Haralambi (February 2019). "Characterising LMC Star cluster NGC 2004". AIP Conference Proceedings. 2075 (1): 090005. Bibcode:2019AIPC.2075i0005N. doi:10.1063/1.5091219. S2CID 126858905. 090005.
  • Media related to NGC 2004 at Wikimedia Commons