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Dwarf irregular galaxy in the constellation of Pegasus From Wikipedia, the free encyclopedia
The Pegasus Dwarf Irregular Galaxy (also known as Peg DIG or the Pegasus Dwarf) is a dwarf irregular galaxy in the direction of the constellation Pegasus. It was discovered by A. G. Wilson in the 1950s. The Pegasus Dwarf is a companion of the Andromeda Galaxy in the Local Group.
Pegasus Dwarf Irregular Galaxy | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Pegasus |
Right ascension | 23h 28m 36.2s[1] |
Declination | +14° 44′ 35″[1] |
Redshift | −183 ± 0 km/s[1] |
Distance | 3.0 ± 0.1 Mly (920 ± 30 kpc)[2] |
Apparent magnitude (V) | 13.2[1] |
Characteristics | |
Type | dIrr/dSph[1][a] |
Apparent size (V) | 5.0′ × 2.7′[1] |
Other designations | |
UGC 12613,[1] PGC 71538,[1] DDO 216,[1] Pegasus Dwarf,[1] PegDIG[1] |
In 1975 Tully & Fisher determined that it was part of the Local Group.[3] The metallicity and the related distance estimate has been subject to discussions in the scientific literature, with varying results; however, recently, by use of the tip of the red-giant branch, a distance within 10% error was achieved in 2000[4][5] and then improved to 3% in 2005.[2]
The science fiction television series Stargate Atlantis takes place in the "Pegasus galaxy" and has shown images of an irregular galaxy. However, the franchise has not explicitly stated if it is the Irregular, Spheroidal, or an entirely fictional location,[6] but since the series claimed the Pegasus galaxy to be 3 million light years away, it is likely the irregular one.
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