NGC 6106 is a spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 1,527±6 km/s, which corresponds to a Hubble distance of 73.5 ± 5.2 Mly (22.52 ± 1.58 Mpc). This is in good agreement with 29 non-redshift measurements which give an average distance of 72.64 ± 2.49 Mly (22.272 ± 0.764 Mpc). It was discovered by German-British astronomer William Herschel on 13 April 1784. NGC 6106 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Luminous red nova and supernova
One luminous red nova and one supernova have been observed in NGC 6106:
AT 2020kog (type LRN, mag. 20.3) was discovered by Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) Search for Kilonovae on 18 May 2020. SN 2024ahv (Type Ib, mag. 16.2) was discovered by Japanese astronomer Hidehiko Okoshi on 16 January 2024.
See also List of NGC objects (6001–7000)
References
External links Media related to NGC 6106 at Wikimedia Commons NGC 6106 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images



