NGC 701

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NGC 701
NGC 0701 SDSS.jpg
NGC 701 imaged by the Sloan Digital Sky Survey
Observation data (J2000 epoch)
Constellation Cetus
Right ascension 01h 51m 03.848s [1]
Declination −09° 42′ 09.32″ [1]
Redshift 0.00611±0.00002 [2]
Helio radial velocity 1831.13±5.10 [2]
Distance 85.6  Mly (26.25  Mpc) [3]
Group or cluster NGC 681 Group [4]
Characteristics
Type SBcd [3]
Other designations
AGC 410368, PGC 6826 [5]

NGC 701 is a spiral galaxy with a high star formation rate in the constellation Cetus. It is estimated to be 86 million light years from the Milky Way and has a diameter of approximately 65,000 light years. The object was discovered on January 10, 1785 by the German-British astronomer William Herschel. [6] [7] [8]

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<span class="mw-page-title-main">NGC 3539</span> Lenticular galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 41</span> Spiral Galaxy in the constellation Pegasus

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<span class="mw-page-title-main">NGC 4866</span> Lenticular galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 100</span> Spiral galaxy located in the constellation Pisces

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<span class="mw-page-title-main">NGC 79</span> Elliptical galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 4138</span> Lenticular galaxy in the constellation Canes Venatici

NGC 4138 is the New General Catalogue identifier for a lenticular galaxy in the northern constellation of Canes Venatici. Located around 52 million light years from Earth, it spans some 2.1 × 1.3 arc minutes and has an apparent visual magnitude of 11.3. The morphological classification of NGC 4138 is SA0+(r), indicating it lacks a bar formation and has tightly wound spiral arms with a ring-like structure around the nucleus. It has no nearby companion galaxies.

<span class="mw-page-title-main">NGC 4178</span> Barred spiral galaxy in the constellation Virgo

NGC 4178 is the New General Catalogue identifier for a barred spiral galaxy in the equatorial constellation of Virgo. It was discovered April 11, 1825 by English astronomer John Herschel. Located some 43.8 million light years away, this galaxy spans 2.3 × 0.4 arc minutes and is seen at a low angle, being inclined by 77° to the line of sight from the Earth. The morphological classification of NGC 4178 is SB(rs)dm, indicating that it has a bar feature at the core, and, per the '(rs)', has traces of a ring-like structure surrounding the bar. The 'dm' suffix indicates the spiral arms are diffuse, broken, and irregular in appearance with no bulge at the nucleus. This galaxy is a member of the Virgo Cluster, which is the richest nearby group of galaxies outside the Local Group and forms the core of the Virgo Supercluster.

<span class="mw-page-title-main">NGC 4203</span> Lenticular galaxy in the constellation Coma Berenices

NGC 4203 is the New General Catalogue identifier for a lenticular galaxy in the northern constellation of Coma Berenices. It was discovered on March 20, 1787 by English astronomer William Herschel, and is situated 5.5° to the northwest of the 4th magnitude star Gamma Comae Berenices and can be viewed with a small telescope. The morphological classification of NGC 4203 is SAB0−, indicating that it has a lenticular form with tightly wound spiral arms and a weak bar structure at the nucleus.

<span class="mw-page-title-main">NGC 5470</span> Spiral galaxy in the constellation Virgo

NGC 5470 is an edge-on spiral galaxy located between 43 and 68 million light-years away in the constellation Virgo. It was discovered by astronomer John Herschel in 1830. It is a member of the Virgo III Groups, a series of galaxies and galaxy clusters strung out to the east of the Virgo Supercluster of galaxies.

<span class="mw-page-title-main">NGC 770</span> Elliptical galaxy in the constellation Aries

NGC 770 is an elliptical galaxy in the constellation Aries. It is around 120 million light years from the Milky Way and has a diameter of around 36,000 ly. NGC 770 is gravitationally linked to NGC 772. The galaxy was discovered on November 3, 1855 by RJ Mitchell.

<span class="mw-page-title-main">NGC 2227</span> Barred spiral galaxy in the constellation Canis Major

NGC 2227 is a barred spiral galaxy with a morphological type of SB(rs)c located in the direction of the Canis Major constellation. It was discovered on January 27, 1835, by John Herschel.

<span class="mw-page-title-main">NGC 546</span> Barred spiral galaxy in the constellation Sculptor

NGC 546 is a barred spiral galaxy about 270 million light years away from Earth and located in the constellation Sculptor. The largest diameter is 1.40 and the smallest is 0.5 angular minutes. The first discovery was made by John Frederick William Herschel on 23 October 1835.

References

  1. 1 2 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN   0004-6256. S2CID   18913331.
  2. 1 2 Koribalski, B. S.; et al. (July 2004). "The 1000 Brightest HIPASS Galaxies: H I Properties". The Astronomical Journal. 128 (1): 16–46. arXiv: astro-ph/0404436 . Bibcode:2004AJ....128...16K. doi:10.1086/421744. S2CID   16229767.
  3. 1 2 Ann, H. B.; et al. (2015). "A Catalog of Visually Classified Galaxies in the Local (z ∼ 0.01) Universe". The Astrophysical Journal Supplement Series. 217 (2): 27–49. arXiv: 1502.03545 . Bibcode:2015ApJS..217...27A. doi:10.1088/0067-0049/217/2/27. S2CID   119253507.
  4. ↑ Tully, R. Brent; et al. (2013). "Cosmicflows-2: The Data". The Astronomical Journal. 146 (4): 86. arXiv: 1307.7213 . Bibcode:2013AJ....146...86T. doi:10.1088/0004-6256/146/4/86. S2CID   118494842.
  5. ↑ "NGC 701". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-01-11.
  6. ↑ Ford, Dominic. "The galaxy NGC 701 - In-The-Sky.org". in-the-sky.org. Retrieved 2019-12-17.
  7. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-12-17.
  8. ↑ "Revised NGC Data for NGC 701". spider.seds.org. Retrieved 2019-12-17.
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