NGC 5406 is a barred spiral galaxy in the constellation of Canes Venatici. Its velocity with respect to the cosmic microwave background is 5,571±13 km/s, which corresponds to a Hubble distance of 268.0 ± 18.8 Mly (82.17 ± 5.76 Mpc). However, seven non-redshift measurements give a much closer mean distance of 140.06 ± 34.21 Mly (42.943 ± 10.489 Mpc). It was discovered by German-British astronomer William Herschel on 16 May 1787. NGC 5406 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms. According to Abraham Mahtessian, NGC 5406 and NGC 5407 form a pair of galaxies.
Supernovae Two supernovae have been observed in NGC 5406:
SN 1977B (type unknown, mag. 14) was discovered by Hungarian Astronomer Miklós Lovas on 18 March 1977. PSN J14002117+3854517 (Type II, mag. 18.2) was discovered by Paolo Campaner and the Italian Supernovae Search Project (ISSP) on 18 February 2015.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5406 at Wikimedia Commons NGC 5406 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


