NGC 676 explained

NGC 676
Credit:NASA
Epoch:J2000
Type:S0/a: edge-on[1]
Dist Ly:18.7abbr=onNaNabbr=on
Z:0.004983±0.000083[2]
Appmag V:10.5 +/- 0.4 [3]
Size V:4.0 × 1.2
Constellation Name:Pisces
Names:UGC 01270; Ark 057;[4] CGCG 412-028; CGCG 0146.3+0540, PGC 6656

NGC 676 is a lenticular[5] Seyfert 2 galaxy about 18.7 Mly away in the constellation Pisces.[1] It 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.

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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. Arakelian . Marat . The Galaxies of High Surface Brightness . Communications of the Byurakan Astrophysical Observatory . January 1975 . 47 . 3–42 . Marat Arakelian. 25 August 2020. 1975CoBAO..47....3A.
  5. Web site: NGC 676 - Lenticular Galaxy . TheSkyLive.com . 23 August 2020 .