Sculptor Dwarf Galaxy

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For the nearby irregular galaxy within the constellation Sculptor, see Sculptor Dwarf Irregular Galaxy.
Sculptor Dwarf Elliptical Galaxy
Observation data (J2000 epoch)
Constellation Sculptor
Right ascension 01h 00m 09.3s[1]
Declination -33° 42′ 33″[1]
Redshift 110 ± 1 km/s[1]
Distance 290 ± 30 kly (90 ± 10 kpc)[2][3]
Type E[1]
Apparent dimensions (V) 39′.8 × 30′.9[1]
Apparent magnitude (V) 10.1[1]
Other designations
Sculptor Dwarf Spheroidal[1] PGC 3589[1]
See also: Galaxy, List of galaxies

The Sculptor Dwarf Galaxy (also called the Sculptor Dwarf Elliptical Galaxy or the Sculptor Dwarf Spheroidal Galaxy) is a dwarf spheroidal galaxy that is a satellite of the Milky Way. The galaxy lies within the constellation Sculptor. It was discovered in 1938 by Harlow Shapley.[citation needed] The galaxy is located about 290,000 light-years away from the solar system.

[edit] Metallacity

In 1999, Majewski et al. determined that the metallicity of Sculptor dwarf appears to be broken up into two distinct groups, one with [Fe/H] = -2.3 and the other with [Fe/H] = -1.5. Similar to many of the other Local Group galaxies, the older metal-poor segment appears more extended than the younger metal-rich segment.[4]

[edit] References

  1. ^ a b c d e f g h NASA/IPAC Extragalactic Database. Results for PGC 3589. Retrieved on 2006-12-03.
  2. ^ I. D. Karachentsev, V. E. Karachentseva, W. K. Hutchmeier, D. I. Makarov (2004). "A Catalog of Neighboring Galaxies" (abstract). Astronomical Journal 127: 2031-2068. doi:10.1086/382905. 
  3. ^ Karachentsev, I. D.; Kashibadze, O. G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics 49 (1): 3-18. doi:10.1007/s10511-006-0002-6. 
  4. ^ van den Bergh, Sidney (April 2000), “Updated Information on the Local Group”, The Publications of the Astronomical Society of the Pacific 112 (770): 529-536, <http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000PASP..112..529V> 

[edit] External links