Coordinates: Sky map 14h 03m 38.7349s, −33° 58′ 41.809″

NGC 5419

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NGC 5419
NGC 5419 imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationCentaurus
Right ascension14h 03m 38.7349s[1]
Declination−33° 58′ 41.809″[1]
Redshift0.013763[1]
Heliocentric radial velocity4126 ± 15 km/s[1]
Distance210.5 ± 14.8 Mly (64.53 ± 4.54 Mpc)[1]
Group or clusterNGC 5488 Group (LGG 369)
Apparent magnitude (V)10.8[1]
Characteristics
TypeE[1]
Size~428,600 ly (131.42 kpc) (estimated)[1]
Apparent size (V)4.1′ × 3.3′[1]
Other designations
2MASX J14033877-3358422, MCG -06-31-019, PGC 50100, ESO 384- G 039[1]

NGC 5419 is a large elliptical galaxy in the constellation of Centaurus. Its velocity with respect to the cosmic microwave background is 4,375 ± 23 km/s, which corresponds to a Hubble distance of 64.5 ± 4.5 Mpc (~210 million light-years).[1] It was discovered by British astronomer John Herschel on 1 May 1834.[2]

NGC 5419 is the brightest cluster galaxy of the galaxy cluster, Abell S0753.[3] It contains a large core with a radius span of 1.58 arcsec (≈55 pc). In addition, it has a double nucleus, indicating the presence of two supermassive black holes in the center with a separation gap of only ≈70 pc.[4][5][6]

Supernovae

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Two supernovae have been observed in NGC 5419:

NGC 5488 Group

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According to A.M. Garcia, the galaxy NGC 5419 is part of the NGC 5488 group (also known as LGG 369). This group of galaxies has 14 members: NGC 5397, NGC 5488, IC 4366 and nine galaxies from the ESO catalog.[9]

See also

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References

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  9. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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  • Error creating thumbnail: File missing Media related to Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). at Wikimedia Commons
  • NGC 5419 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images