NGC 3079

Background

NGC 3079 was discovered by German-British astronomer William Herschel on 1 April 1790. It is classified as a Seyfert II galaxy, meaning its nucleus has very high surface brightness and strong, high-ionization emission lines, yet the host galaxy is clearly visible. The galaxy's most striking feature is a lumpy bubble of hot gas at its center, imaged by the Hubble Space Telescope.

This bubble is about 3,000 light-years wide and rises more than 3,500 light-years above the galactic disk. It is thought to have been created about one million years ago by particles streaming at high speeds, resulting from a large burst of star formation. Computer modeling suggests an ongoing cycle, with a new bubble forming approximately every 10 million years.

NGC 3079 is the namesake of the NGC 3079 Group (LGG 188), which includes six galaxies: NGC 3073, UGC 5421, UGC 5479, UGC 5459, and UGC 5460. NGC 3079 and NGC 3073 are also listed together as Holm 156 in Erik Holmberg's 1937 study of double and multiple galaxies. Two supernovae have been observed in NGC 3079: SN 2001ci (Type Ic, magnitude 18.3) discovered on 17 April 2001 by LOTOSS, and SN 2013ee (Type II, magnitude 15.5) discovered by Giancarlo Cortini on 13 July 2013.