NGC 676 is a lenticular Seyfert 2 galaxy in the constellation Pisces. Its velocity with respect to the cosmic microwave background is 1217 ± 20 km/s, which corresponds to a Hubble distance of 58.6 ± 4.2 Mly (17.96 ± 1.29 Mpc). In addition, two non redshift measurements give a distance of 61.0 ± 2.6 Mly (18.7 ± 0.8 Mpc). The galaxy was discovered by German-British astronomer William Herschel on 30 September 1786. 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. It is one of the 621 galaxies described in Marat Arakelian's catalog of high-surface-brightness galaxies.
Image Gallery
See also Spiral galaxy List of NGC objects (1–1000)
References
External links Media related to NGC 676 at Wikimedia Commons
NGC 676 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images Students for the Exploration and Development of Space - NGC 676 Telescopius - NGC 676 SkyMap.org - NGC 676 NGC 676 on SIMBAD



