NGC 5939 explained

NGC 5939
Constellation Name:Ursa Minor
Epoch:J2000
Type:S?[1]
Dist Ly:NaNMpc
Z:0.022235
H Radial V:6666 ± 4 km/s
Appmag V:13.1
Size V:0.9' x 0.5'
Size:~31.44kpc (estimated)

NGC 5939 is a spiral galaxy in the constellation of Ursa Minor. Its velocity with respect to the cosmic microwave background is 6684 ± 4 km/s, which corresponds to a Hubble distance of 98.59 ± 6.90 Mpc (∼322 million light-years). It was discovered by American astronomer Lewis Swift on 11 July 1883.[2]

Supernovae

Three supernovae have been observed in NGC 5939: SN 2004ax (type Ib/c, mag. 17.7),[3] [4] SN 2019gss (type II, mag. 19.3),[5] and SN 2023gps (type Ia, mag. 20).[6]

NGC 5939 Group

NGC 5939 is part of a trio of galaxies: The other two galaxies in the group are IC 1129 and UGC 9896.[7]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 5939 . 10 August 2024.
  2. Web site: NGC 5939. Seligman . Courtney . Celestial Atlas . 10 August 2024 .
  3. Web site: Transient Name Server . Entry for SN 2004ax . 10 August 2024.
  4. Web site: Central Bureau for Astronomical Telegrams . Green . Daniel W. E. . Circular No. 8331. April 24, 2004 . 8 August 2024.
  5. Web site: Transient Name Server . Entry for SN 2019gss . 10 August 2024.
  6. Web site: Transient Name Server . Entry for SN 2023gps . 10 August 2024.
  7. Mahtessian . Abraham . Groups of galaxies. III. Some empirical characteristics . July 1998 . Astrophysics . 41 #3 . 308-321 . 10.1007/BF03036100 . 10 August 2024.