NGC 5334 explained

NGC 5334
Epoch:J2000
Constellation Name:Virgo
Type:SB(rs)c[1]
Dist Ly:NaNMpc
Z:0.004623
H Radial V:1386 ± 3 km/s
Appmag V:14.3
Size:~43.62kpc (estimated)
Size V:1.9 × 1.3

NGC 5334 is a face-on barred spiral galaxy in the constellation Virgo. Its velocity with respect to the cosmic microwave background is 1668 ± 20km/s, which corresponds to a Hubble distance of NaNMpc. However, five non-redshift measurements give a distance of NaNMpc.[2] It was discovered by German-British astronomer William Herschel on 15 April 1787.[3] It was also observed by American astronomer Lewis Swift on 20 April 1897 and listed in the Index Catalogue as IC 4338.

NGC 5334 is a member of the Virgo III Groups, a series of galaxies and galaxy clusters strung out to the east of the Virgo Supercluster of galaxies.[4]

Although no supernovae have been observed in NGC 5334 yet, a luminous blue variable, designated SN2003gm (type LBV, mag. 17), was discovered on 6 July 2003.[5] [6]

See also

External links

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 5334 . 2007-04-06 .
  2. Web site: Distance Results for NGC5334 . NASA/IPAC EXTRAGALACTIC DATABASE . . 23 November 2024.
  3. Web site: New General Catalogue Objects: NGC5334 . Seligman . Courtney . Celestial Atlas . 23 November 2024.
  4. Web site: The Virgo III Groups . Atlas of the Universe . 2010-11-27 .
  5. Web site: Transient Name Server . SN2003gm . . 23 November 2024.
  6. Web site: Circular No. 8167 . Green . Daniel W. E. . 27 July 2003 . Central Bureau for Astronomical Telegrams . Dept. of Earth and Planetary Sciences, Harvard University . 23 November 2024.