NGC 908

Source: Wikipedia, the free encyclopedia.
UGCA 27, MCG -04-06-035, PGC 9057[2]

NGC 908 is an

light years away from Earth. It is the main galaxy in the NGC 908 group, which also includes NGC 899, NGC 907, and IC 223.[3]

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.[4]

Two supernovae have been observed in NGC 908: SN 1994ai (type Ic, mag. 17)[5] and SN 2006ce (type Ia, mag. 12.4).[6][7]

References

  1. ^ a b c d e f "Results for NGC 908". NASA/IPAC Extragalactic Database. Retrieved 2006-11-18.
  2. ^ a b "Your NED Search Results". NASA/IPAC Extragalactic Database. Retrieved 2020-11-09.
  3. S2CID 119194025. Archived from the original
    on 31 January 2016. Retrieved 1 January 2016.
  4. ^ "The Starburst Galaxy NGC 908". ESO. 26 July 2006. Retrieved 9 November 2020.
  5. ^ Transient Name Server entry for SN 1994ai. Retrieved 30 March 2023.
  6. IAU
    Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
  7. ^ Transient Name Server entry for SN 2006ce. Retrieved 30 March 2023.

External links