NGC 839

In today's world, NGC 839 has gained unprecedented relevance. Since its emergence, NGC 839 has significantly impacted various aspects of society, culture and economy. In this article, we will thoroughly explore the impact of NGC 839 and its influence in different areas of daily life. We will analyze its evolution over time, its implications in terms of social and political changes, as well as the opportunities and challenges it poses for the future. Through detailed analysis, we will examine the importance of understanding and reflecting on NGC 839 to be better prepared for the challenges of the contemporary world.

NGC 839
HST image of NGC 839
Observation data (J2000 epoch)
ConstellationCetus
Right ascension02h 09m 42.929s[1]
Declination−10° 11′ 02.71″[1]
Redshift0.012916[2]
Heliocentric radial velocity3847 km/s[2]
Distance174.3 ± 12.2 Mly (53.44 ± 3.75 Mpc)[1]
Apparent magnitude (V)11.42[2]
Apparent magnitude (B)13.98[2]
Characteristics
TypeS0: pec[1]
Other designations
MCG -02-06-034, PGC 8254[2]

NGC 839 is a lenticular galaxy located in the constellation Cetus. It was discovered November 28, 1785 in a sky survey by Wilhelm Herschel.[3] It is one of the galaxies that are part of the quadruplet family HGC 16, along with the unbarred lenticular galaxy NGC 838.[2]

NGC 839 is a luminous infrared galaxy (LIRG) that shows signs of high amounts of star formation; therefore, it is also classified as a starburst galaxy.[4] It is similar in appearance to Messier 82, suggesting a similar formation history.[4]

References

  1. ^ a b c d "Results for object NGC 0839 (NGC 839)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-09-08.
  2. ^ a b c d e f "NGC 839". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-09-08.
  3. ^ Seligman, Courtney. "New General Catalogue objects: NGC 800 - 849". cseligman.com. Retrieved 2021-09-08.
  4. ^ a b Rich, J. A.; Dopita, M. A.; Kewley, L. J.; Rupke, D. S. N. (2010). "NGC 839: Shocks in an M82-like Superwind". The Astrophysical Journal. 721 (1): 505–517. arXiv:1007.3495. Bibcode:2010ApJ...721..505R. doi:10.1088/0004-637X/721/1/505. S2CID 118875933.