NGC 5630 explained

NGC 5630
Constellation Name:Boötes
Epoch:J2000
Type:Sdm?[1]
Dist Ly:NaNMpc
Z:0.008918
H Radial V:2673 ± 2 km/s
Appmag V:13.0
Size V:2.2' x 0.7'
Size:~23.21kpc (estimated)

NGC 5630 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 2826 ± 11 km/s, which corresponds to a Hubble distance of 41.68 ± 2.92 Mpc (∼136 million light-years). It was discovered by German-British astronomer William Herschel on 9 April 1787.[2]

NGC 5630 is listed as a field galaxy, i.e. one does not belong to a larger galaxy group or cluster and hence is gravitationally alone.[3]

Three supernovae have been observed in NGC 5630: SN 2005dp (type II, mag. 16),[4] [5] SN 2006am (type IIn, mag. 18.5),[6] and SN 2023zdx (Type II-P, mag. 17).[7]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 5630 . 8 August 2024.
  2. Web site: Celestial Atlas entry for NGC 5630. Seligman . Courtney . cseligman.com . 8 August 2024 .
  3. 1976ApJS...32..409T. Groups of galaxies. I. A catalog. Turner. E. L.. Gott, J. R., III. The Astrophysical Journal Supplement Series. 1976. 32. 409. 10.1086/190403.
  4. Web site: Transient Name Server . Entry for SN 2005dp . 8 August 2024.
  5. Web site: Central Bureau for Astronomical Telegrams . Green . Daniel W. E. . Circular No. 8594 . September 3, 2005 . 8 August 2024.
  6. Web site: Transient Name Server . Entry for SN 2006am . 8 August 2024.
  7. Web site: Transient Name Server . Entry for SN 2023zdx . 8 August 2024.