NGC 908

NGC 908 is an unbarred spiral galaxy in the constellation Cetus. It is 60 million light years away from Earth. NGC 908 has vigorous star formation and is a starburst galaxy. The galaxy has a three-arm spiral pattern; two of its arms have peculiar morphology. The galaxy has a bright central bulge. Clusters of young stars and star-forming knots can be seen in the arms. Starburst activity and the peculiar morphology of the galaxy indicate it had a close encounter with another galaxy, although none are visible now.[3] NGC 908 was discovered in 1786 by William Herschel. Two supernovae have been observed in NGC 908, SN 1994ai (Ic type, mag. 17) and SN 2006ce (Ia type, mag. 12.4).[4] It is the main galaxy in the NGC 908 group, which also includes NGC 899, NGC 907, and IC 223.[5]

NGC 908
NGC 908 by the Very Large Telescope of ESO.
Credit: NASA/STScI/WikiSky
Observation data (J2000 epoch)
ConstellationCetus
Right ascension02h 23m 04.6s[1]
Declination−21° 14′ 02″[1]
Redshift1509 ± 5 km/s[1]
Distance56.0 ± 5.7 Mly (17.2 ± 1.8 Mpc)[1]
Apparent magnitude (V)10.83[2]
Characteristics
TypeSA(s)c [1]
Apparent size (V)6′.0 × 2′.6[1]
Other designations
MCG-04-06-035, PGC 9057[2]

References
  1. "Results for NGC 908". NASA/IPAC Extragalactic Database. Retrieved 2006-11-18.
  2. "Your NED Search Results". NASA/IPAC Extragalactic Database. Retrieved 2020-11-09.
  3. "The Starburst Galaxy NGC 908". ESO. 26 July 2006. Retrieved 9 November 2020.
  4. "List of Supernovae". IAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
  5. Dmitry Makarov and Igor Karachentsev (2011). "Galaxy groups and clouds in the local (z∼ 0.01) Universe". MNRAS. 412 (4): 2498–2520. arXiv:1011.6277. Bibcode:2011MNRAS.412.2498M. doi:10.1111/j.1365-2966.2010.18071.x. Retrieved 1 January 2016.
  • Media related to NGC 908 at Wikimedia Commons


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.