NGC 5090 and NGC 5091
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NGC 5090 and NGC 5091 are a set of galaxies approximately Script error: No such module "convert". away in the constellation Centaurus.[1] They are in the process of colliding and merging with some evidence of tidal disruption of NGC 5091.[2]
NGC 5090 is an elliptical galaxy while NGC 5091 is a barred spiral galaxy.[1] The radial velocity of the nucleus of NGC 5090 has been measured at Template:Cvt, while NGC 5091 has a radial velocity of Template:Cvt.[2] NGC 5090 is associated with the strong, double radio source PKS 1318-43.[2]
Two supernovae have been observed in NGC 5090:
- SN 1981C (type unknown, mag. 14.5) was discovered by José Maza on 2 March 1981.[3][4]
- SN 2025cy (typeScript error: No such module "String".Ia, mag. 18.03) was discovered by BlackGEM on 1 January 2025.[5]
See also
References
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External links
- "Of Holes in the Sky and Pretty Galaxies" by the European Southern Observatory
- Template:APOD
- Template:WikiSky