NGC 6195 is a large spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 9,005±3 km/s, which corresponds to a Hubble distance of 433.2 ± 30.3 Mly (132.82 ± 9.30 Mpc). Additionally, four non-redshift measurements give a farther mean distance of 466.40 ± 13.64 Mly (143.000 ± 4.183 Mpc). It was discovered by German-British astronomer William Herschel on 30 May 1791. NGC 6195 is a Seyfert I galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable. It is also a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
Abell 2199 cluster NGC 6195 is a member of the galaxy cluster Abell 2199.
Supernova One supernova has been observed in NGC 6195:
SN 1975K (type unknown, mag. 17.8) was discovered by American astronomer Charles Kowal on 9 August 1975.
See also List of NGC objects (6001–7000)
References
External links Media related to NGC 6195 at Wikimedia Commons NGC 6195 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


