NGC 454

Pair of interacting galaxies in the constellation Phoenix From Wikipedia, the free encyclopedia

NGC 454 is a pair of interacting galaxies located 150 million light years away in the constellation Phoenix. John Herschel discovered it on October 5, 1834. It was described by Dreyer as "very faint, small, round, brighter middle."[2] NGC 454 consists of a large elliptical galaxy that had been destroyed by the merging. And the pair also contains a bluish gas-rich irregular galaxy. The irregular galaxy may also have caused a trail of hot blue stars in the right of the image. The elliptical galaxy is on the left and the irregular galaxy is on the right. The trail is also located on the right.

Right ascension01h 14m 22.5s[1]
Declination−55° 23 55[1]
Redshift0.012158[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 454
NGC 454
NGC 454 as seen by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationPhoenix
Right ascension01h 14m 22.5s[1]
Declination−55° 23 55[1]
Redshift0.012158[1]
Heliocentric radial velocity3,645 km/s[1]
Apparent magnitude (V)13.12[1]
Absolute magnitude (V)-20.31[1]
Characteristics
TypeIrr pec? (PGC 4461) and S0 pec? (PGC 4468)[1]
Apparent size (V)1.8' × 1.8'[1]
Other designations
IRAS F01123-5539, PGC 4468[1]
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References

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