Sculptor Group

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Sculptor group

The Sculptor Galaxy (NGC 253), as seen at near-infrared wavelengths. Credit: 2MASS.
Observation data (Epoch J2000)
Constellation(s) Sculptor/Cetus
Right ascension 00h 48m[1]
Declination −25° 17′[1]
Brightest member Sculptor Galaxy (NGC 253)[2][3][4]
Number of galaxies 13[2][3]
Other designations
NGC 253 Group, LGG 4, Sculptor Filament,[3]
South Polar Group, South Galactic Pole Group[4]
See also: Galaxy groups, Galaxy clusters, List of galaxy clusters

The Sculptor Group is a loose group of galaxies[2][3] near the south galactic pole.[1] The group is one of the closest groups of galaxies to the Local Group; the distance to the center of the group from the Milky Way is approximately 3.9 Mpc (12.7 Mly).[3]

The Sculptor Galaxy (NGC 253) and a few other galaxies form a gravitationally-bound core in the center of this group. A few other galaxies at the periphery may be associated with the group but may not be gravitationally bound. Because most of the galaxies in this group are actually weakly gravitationally bound, the group may also be described as a filament.[2][3]

Members

The table below lists galaxies that have been identified as associated with the Sculptor Galaxy (and hence associated with the group) by I. D. Karachentsev and collaborators.[2][3]

Members of the Sculptor Group
Name Type[5] R.A. (J2000)[5] Dec. (J2000)[5] Redshift (km/s)[5] Apparent Magnitude[5]
IC 1574 IM(s)m 00h 43m 03.8s −22° 14′ 49″ 363 ± 4 15.1
NGC 59 SA(rs)0 00h 15m 25.1s −21° 26′ 39.8″ 362 ± 10 13.1
NGC 247 SAB(s)d 00h 47m 08.5s −20° 45′ 37″ 156 ± 2 9.9
NGC 625 SB(s)m 01h 35m 04.6s −41° 26′ 10″ 396 ± 1 11.7
NGC 7793 SA(s)d 23h 57m 49.8s −32° 35′ 28″ 227 ± 2 10.0
PGC 2881 IABm 00h 49m 20.9s −18° 04′ 32″ 16.5
PGC 2933 IAB(s)m pec 00h 50m 24.3s −19° 54′ 24″ 16.6
PGC 6430 IB(s)m 01h 45m 03.7s −43° 35′ 53″ 391 ± 2 12.7
Sculptor-dE1 dE 00h 23m 51.7s −24° 42′ 18″ 16.9
Sculptor Dwarf Irregular Galaxy
(PGC 621)		 IBm 00h 08m 13.4s −34° 34′ 42″ 221 ± 6 15.5
Sculptor Galaxy
(NGC 253)		 SAB(s)c 00h 47m 33.1s −25° 17′ 18″ 243 ± 2 8.0
UGCA 15 IB(s)m 00h 49m 49.2s −21° 00′ 54″ 295 ± 0 15.2
UGCA 442 SB(s)m 23h 43m 45.5s −31° 57′ 24″ 267 ± 2 13.6

Note that the object names used in the above table differ from the names used by Karachentsev and collaborators. NGC, IC, UGC, and PGC numbers have been used when possible to allow for easier referencing.

Foreground galaxies

The irregular galaxy NGC 55, the spiral galaxy NGC 300, and their companion galaxies have been considered by many researchers to be part of this group. However, recent distance measurements to these and other galaxies in the same region of the sky show that NGC 55, NGC 300, and their companions may simply be foreground galaxies that are physically unassociated with the Sculptor Group.[2]

References

  1. ↑ 1.0 1.1 1.2 "NASA/IPAC Extragalactic Database". Results for NGC 253, identified as the core of the Sculptor Group. Retrieved 2006-11-25. 
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 I. D. Karachentsev, E. K. Grebel, M. E. Sharina, A. E. Dolphin, D. Geisler, P. Guhathakrta, P. W. Hodge, V. E. Karachentseva, A. Sarajedini, P. Seitzer (2003). "Distances to nearby galaxies in Sculptor". Astronomy and Astrophysics 404 (1): 93–111. arXiv:astro-ph/0302045. Bibcode:2003A&A...404...93K. doi:10.1051/0004-6361:20030170. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 I. D. Karachentsev (2005). "The Local Group and Other Neighboring Galaxy Groups". Astronomical Journal 129 (1): 178–188. arXiv:astro-ph/0410065. Bibcode:2005AJ....129..178K. doi:10.1086/426368. 
  4. ↑ 4.0 4.1 Burnham, Robert (1978). Burnham's Celestial Handbook; An Observers Guide to the Universe Beyond the Solar System; Volume Three, Pavo Through Vulpecula. Dover Publications, Inc. p. 1736. ISBN 0-486-24065-7. 
  5. ↑ 5.0 5.1 5.2 5.3 5.4 "NASA/IPAC Extragalactic Database". Results for various galaxies. Retrieved 2006-11-25. 

Coordinates: 00h 48m 00s, −25° 17′ 00″

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