NGC 6308 explained

NGC 6308
Constellation Name:Hercules
Epoch:J2000
Type:SAB(rs)c?[1]
Dist Ly:NaNMpc
Z:0.029402
H Radial V:8814 ± 3 km/s
Appmag V:13.4
Size V:1.1' x 1.0'
Size:~60.89kpc (estimated)

NGC 6308 is a large intermediate spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 8797 ± 3 km/s, which corresponds to a Hubble distance of 129.74 ± 9.08 Mpc (∼423 million light-years). It was discovered by German astronomer Albert Marth on 6 June 1863.[2]

NGC 6308 has been identified as an isolated galaxy, i.e. it does not belong to a cluster or group.[3]

One supernova has been observed in NGC 6308: SN 2023oyz (type Ic, mag 20.4).[4]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 6308 . 6 August 2024.
  2. https://cseligman.com/text/atlas/ngc63.htm#6308 Celestial Atlas entry for NGC 6308.
  3. https://ui.adsabs.harvard.edu/abs/1986A%26A...154..343V/abstract Isolated galaxies. By Vettolani, G. ; de Souza, R. ; Chincarini, G. Astronomy and Astrophysics, Vol. 154, p. 343-348 (1986)
  4. https://www.wis-tns.org/object/2023oyz Transient Name Server entry for SN 2023oyz.