- Source: NGC 1278
NGC 1278 is an elliptical galaxy located about 230 million light-years away in the constellation Perseus. NGC 1278 was discovered by astronomer Heinrich d'Arrest on February 14, 1863. It was then rediscovered by astronomer Guillaume Bigourdan on October 22, 1884 and was later listed as IC 1907. NGC 1278 is a member of the Perseus Cluster and is a low-luminosity AGN (LLAGN).
One supernova, SN 2016ajf (type Ia, mag. 16.9), was discovered in NGC 1278 on 18 February, 2016.
Globular clusters
Unlike the nearby galaxy NGC 1277 which has a dominant population of metal-rich or “red” globular clusters, NGC 1278 has a rich population of both metal-rich and metal-poor or “blue” globular clusters.
See also
List of NGC objects (1001–2000)
NGC 1275
NGC 1277
References
External links
Media related to NGC 1278 at Wikimedia Commons
NGC 1278 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Kata Kunci Pencarian:
- NGC 1277
- Messier 22
- Sistem Data Astrofisika
- Daftar bintang di rasi bintang Cassiopeia
- Daftar bintang di rasi bintang Norma
- NGC 1278
- List of NGC objects (1001–2000)
- Omega Nebula
- List of IC objects
- Messier 22
- List of largest star clusters
- NGC 1624-2
- NGC 2080
- Cygnus X-1
- Astrophysics Data System
