Sagittarius Dwarf Irregular Galaxy

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Not to be confused with the Sagittarius Dwarf Elliptical Galaxy.
SagDIG
SagDIG.jpg
Observation data (J2000 epoch)
Constellation Sagittarius
Right ascension 19h 29m 59.0s[1]
Declination −17° 40′ 41″[1]
Redshift -79 ± 1 km/s[1]
Distance 3.39 ± 0.23 Mly (1.04 ± 0.07 Mpc)[2][3]
Type IB(s)m[1] V (Dwarf irregular galaxy)
Apparent dimensions (V) 2′.9 × 2′.1[1]
Apparent magnitude (V) 15.5[1]
Other designations
Sagittarius Dwarf Irregular,[1] SGR Dwarf,[1]
ESO594-G004,[1] PGC 63287,[1] Kowal's Object[1]
See also: Galaxy, List of galaxies

The Sagittarius Dwarf Irregular Galaxy or SagDIG is a dwarf galaxy in the constellation of Sagittarius. It lies about 3.4 million light-years away. SagDIG should not be confused with the Sagittarius Dwarf Elliptical Galaxy or SagDEG, a satellite galaxy of the Milky Way. It was discovered by Cesarsky et al. on a photographic plate taken for the ESO (B) Atlas on June 13, 1977 using the ESO 1 meter Schmidt telescope.

The SagDIG is the most remote object from the barycenter thought to be a member of the Local Group. It is only slightly outside the zero-velocity surface of the Local Group.[4]

SagDIG is a much more luminous galaxy than Aquarius Dwarf and it has been through a prolonged star formation (Momany et al. 2005). This has resulted in it containing a rich intermediate-age population of stars. Twenty-seven candidate carbon stars have been identified inside SagDIG. Analysis shows that the underlying stellar population of SagDIG is metal-poor (at least [Fe/H] ≤ −1.3). Further, the population is young, with the most likely average age between 4 and 8 billion years for the dominant population.[5]

References

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External links

Coordinates: Sky map 19h 29m 59.0s, −17° 40′ 41″