NGC 4945 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Centaurus |
Right ascension | 13h 05m 27.5s[1] |
Declination | −49° 28′ 06″[1] |
Redshift | 563 ± 3 km/s[1] |
Distance | 11.7 Mly (3.6 Mpc)[2] |
Apparent magnitude (V) | 9.3[1] |
Characteristics | |
Type | SB(s)cd[1] |
Apparent size (V) | 20.0′ × 3.8′[1] |
Other designations | |
PGC 45279,[1] Caldwell 83 |
NGC 4945 (also known as Caldwell 83) is a barred spiral galaxy in the constellation Centaurus, visible near the star Xi Centauri.[3] The galaxy was discovered by James Dunlop in 1826 and is thought to be similar to the Milky Way Galaxy, although X-ray observations show that NGC 4945 has an unusual energetic Seyfert 2 nucleus that might house a supermassive black hole.[4] Around the nucleus of the galaxy, there is a dense disk of dust and gas, along with many dense star clusters.[5] This object has an estimated mass of 1.4+1.4
−0.7×1011 M☉.[6]
Two supernovae have been observed in NGC 4945: SN 2005af (Type II, mag. 12.8),[7] and SN 2011ja (type IIP, mag. 14).[8]
ned
was invoked but never defined (see the help page).karachentsevetal2002
was invoked but never defined (see the help page).docdb
was invoked but never defined (see the help page).sciday
was invoked but never defined (see the help page).Graham2008
was invoked but never defined (see the help page).