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NGC 3840
SDSS image of NGC 3840
Observation data ( J2000 epoch)
Constellation Leo
Right ascension11h 43m 58.9s [1]
Declination20° 04′ 37″ [1]
Redshift0.024590 [1]
Heliocentric radial velocity7372 km/s [1]
Distance318  Mly (97.5  Mpc) [1]
Group or cluster Leo Cluster
Apparent magnitude (V)14.54 [1]
Characteristics
TypeSa [1]
Size~105,400  ly (32.32  kpc) (estimated) [1]
Apparent size (V)1.1 x 0.8 [1]
Other designations
CGCG 97-91, IRAS 11413+2021, MCG 3-30-70, PGC 36477, UGC 6702 [1]

NGC 3840 is a spiral galaxy [2] located about 320 million light-years away [3] in the constellation Leo. [4] The galaxy was discovered by astronomer Heinrich d'Arrest on May 8, 1864. [5] NGC 3840 is a member of the Leo Cluster. [6] [7] [8] The galaxy is rich in neutral atomic hydrogen (H I) and is not interacting with its environment. [9]

NGC 3840 is likely to be a low-luminosity AGN (LLAGN). [10]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 3840. Retrieved 2018-07-12.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-07-12.
  3. ^ "NED Query Results for NGC 3840". ned.ipac.caltech.edu. Retrieved 2018-07-12.
  4. ^ "Revised NGC Data for NGC 3840". spider.seds.org. Retrieved 2018-07-12.
  5. ^ "New General Catalog Objects: NGC 3800 - 3849". cseligman.com. Retrieved 2018-07-09.
  6. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-07-12.
  7. ^ "NGC 3840". Retrieved 2018-07-12.
  8. ^ "Hierarchy catalogue". leda.univ-lyon1.fr. Retrieved 2018-07-12.
  9. ^ Scott, T. C.; Bravo-Alfaro, H.; Brinks, E.; Caretta, C. A.; Cortese, L.; Boselli, A.; Hardcastle, M. J.; Croston, J. H.; Plauchu, I. (2010-04-11). "Probing evolutionary mechanisms in galaxy clusters: neutral atomic hydrogen in Abell 1367". Monthly Notices of the Royal Astronomical Society. 403 (3): 1175–1192. arXiv: 1001.3900. Bibcode: 2010MNRAS.403.1175S. doi: 10.1111/j.1365-2966.2009.16204.x. ISSN  0035-8711. S2CID  17147621.
  10. ^ Sun, M.; Vikhlinin, A.; Forman, W.; Jones, C.; Murray, S. S. (2005). "The Survival and Destruction of X-Ray Coronae of Early-Type Galaxies in Rich Cluster Environments: A Case Study of A1367". The Astrophysical Journal. 619 (1): 169–177. arXiv: astro-ph/0408425. Bibcode: 2005ApJ...619..169S. doi: 10.1086/425298. ISSN  0004-637X. S2CID  16811452.

External links