NGC 2959 explained

NGC 2959
Constellation Name:Ursa Major
Epoch:J2000
Type:(R')SAB(rs)ab pec, Sa[1]
Dist Ly:66.7Mpc
Z:0.01482
H Radial V:4442 km/s
Appmag V:12.8
Size V:1.4' x 1.4'
Size:~34.3kpc (estimated)

NGC 2959 is an intermediate spiral galaxy in the constellation Ursa Major. Its velocity relative to the cosmic microwave background is 4,525 ± 6 km/s, which corresponds to a Hubble distance of 66.7 ± 4.7 Mpc (~218 million light years.). NGC 2959 was discovered by British astronomer John Herschel on 28 October 1831.

NGC 2959 has a luminosity class of I-II and a broad H I line.

According to the Simbad database, NGC 2959 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[2]

Two supernovae have been observed in NGC 2959: SN 2021bbm (type II, mag. 17.4),[3] and SN 2023vog (type II, mag. 18.5).[4]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 2959 . October 30, 2023.
  2. https://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+2959 SIMBAD: NGC 2959 LINER-type Active Galaxy Nucleus
  3. https://www.wis-tns.org/object/2021bbm Transient Name Server entry for SN 2021bbm.
  4. https://www.wis-tns.org/object/2023vog Transient Name Server entry for SN 2023vog.