NGC 5253

Galaxy in the M83 group of galaxies From Wikipedia, the free encyclopedia

NGC 5253 is an irregular galaxy in the constellation Centaurus. It was discovered by William Herschel on 15 March 1787.[4][5]

Right ascension13h 39m 55.9561s[2]
Declination−31° 38 24.364[2]
Redshift407 ± 3 km/s[2]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 5253
NGC 5253 is one of the nearest of the known Blue Compact Dwarf (BCD) galaxies[1]
Observation data (J2000 epoch)
ConstellationCentaurus
Right ascension13h 39m 55.9561s[2]
Declination−31° 38 24.364[2]
Redshift407 ± 3 km/s[2]
Distance10.9 ± 0.6 Mly (3.33 ± 0.17 Mpc)[3]
Apparent magnitude (V)10.9[2]
Characteristics
TypeIm pec[2]
Size27,300 ly (8.37 kpc) (estimated)[2]
Apparent size (V)5.0 × 1.9[2]
Other designations
Haro 10, ESO 445- G 004, IRAS 13370-3123, UGCA 369, MCG -05-32-060, PGC 48334 [2]
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Properties

NGC 5253 is located within the M83 Subgroup of the Centaurus A/M83 Group, a relatively nearby galaxy group that includes the radio galaxy Centaurus A and the spiral galaxy M83 (the Southern Pinwheel Galaxy). NGC 5253 is considered a dwarf starburst galaxy[6] and also a blue compact galaxy.[7]

Supernovae

Two supernovae have been observed in NGC 5253:

Contents

NGC 5253 contains a giant dust cloud hiding a cluster (believed to be a super star cluster) of more than one million stars, among them up to 7,000 O-type stars. The cluster is 3 million years old and has a total luminosity of more than one billion suns. It is the site of efficient star formation, with a rate at least 10 times higher than comparable regions in the Milky Way.[15][16]

References

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