NGC 676 explained

NGC 676
Epoch:J2000
Type:S0/a: edge-on[1]
Dist Ly:18.7abbr=onNaNabbr=on
Z:0.005023[2]
Appmag V:10.5 +/- 0.4 [3]
Size V:4.0 × 1.2
Size:~27.2kpc (estimated)
Constellation Name:Pisces

NGC 676 is a lenticular[4] Seyfert 2 galaxy in the constellation Pisces.[1] Its velocity with respect to the cosmic microwave background is 1217 ± 20km/s, which corresponds to a Hubble distance of NaNMpc. In addition, two non redshift measurements give a distance of NaNabbr=onNaNabbr=on.[5] The galaxy was discovered by German-British astronomer William Herschel on 30 September 1786.[6]

NGC 676 can be seen near the star α Piscium. Located close to the celestial equator, it is visible from both hemispheres. BD +04 0244, a star with a visual magnitude of 10.44, is superposed 5.1 arc seconds south-southwest of the nucleus.[1] It is one of the 621 galaxies described in Marat Arakelian's catalog of high-surface-brightness galaxies.

See also

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Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 676 . 22 August 2020.
  2. Paturel . G . Dubois . P . Petit . C . Woelfel . F . Comparison LEDA/SIMBAD . LEDA . 24 August 2020 . January 2002. 2002LEDA.........0P .
  3. Web site: NGC 676 . SIMBAD . The Centre de Données Astronomiques de Strasbourg (CDS) . 23 August 2020.
  4. Web site: NGC 676 - Lenticular Galaxy . TheSkyLive.com . 23 August 2020 .
  5. Web site: Distance Results for NGC676 . NASA/IPAC EXTRAGALACTIC DATABASE . . 14 November 2024.
  6. Web site: NGC676 . Seligman . Courtney . Celestial Atlas . 14 November 2024 .