NGC 664 explained

NGC664
Constellation Name:Pisces
Epoch:J2000
Type:Sb?[1]
Dist Ly:NaNMpc
Group Cluster:NGC 664 Group
Z:0.018113
H Radial V:5430 ± 3 km/s
Appmag V:12.8
Size V:1.1' x 0.9'
Size:~35.14kpc (estimated)

NGC664 is a spiral galaxy in the constellation of Pisces. Its velocity with respect to the cosmic microwave background is 5137 ± 21km/s, which corresponds to a Hubble distance of NaNMpc. In addition, six non redshift measurements give a distance of NaNabbr=onNaNabbr=on.[2] It was discovered by British astronomer John Herschel on 24 September 1830.[3]

Supernovae

Three supernovae have been observed in NGC664: SN1996bw (typeII, mag.17.5),[4] SN1997W (type II, mag.18),[5] and SN1999eb (typeIIn, mag.16.2).[6]

NGC 664 Group

NGC 664 is the namesake of the four member NGC664 group. The other three galaxies are: IC 150, UGC 1204, and UGC 1240.[7]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 664 . 22 August 2024.
  2. Web site: Distance Results for NGC664 . NASA/IPAC EXTRAGALACTIC DATABASE . . 22 August 2024.
  3. Web site: NGC664 . Seligman . Courtney . Celestial Atlas . 22 August 2024 .
  4. Web site: Transient Name Server . SN1996bw . . 22 August 2024.
  5. Web site: Transient Name Server . SN1997W . . 22 August 2024.
  6. Web site: Transient Name Server . SN1999eb . . 22 August 2024.
  7. 10.1086/305355 . The Properties of Poor Groups of Galaxies. I. Spectroscopic Survey and Results . 1998 . Zabludoff . Ann I. . Mulchaey . John S. . The Astrophysical Journal . 496 . 1 . 39–72 . astro-ph/9708132 . 1998ApJ...496...39Z .