NGC 644

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NGC 644
NGC 644 DECam.jpg
DECam image of NGC 644
Observation data (J2000 epoch)
Constellation Phoenix
Right ascension 01h 38m 52.975s [1]
Declination −42° 35 07.19 [1]
Redshift 0.020731 [2]
Heliocentric radial velocity 6151 km/s [2]
Distance 268.8  Mly (82.41  Mpc) [3]
Apparent magnitude  (B)14.79 [2]
Characteristics
Type SB(r)bc: [4]
Size126.8  kly (38.88  kpc) [4]
Other designations
MCG -07-04-027, PGC 6097 [2]

NGC 644 is a barred spiral galaxy in the constellation Phoenix in the southern sky. It is estimated to be 270 million light-years from the Milky Way and has a diameter of approximately 130,000 light-years. [4] Together with NGC 641, it probably forms a gravitationally bound pair of galaxies. The object was discovered on September 5, 1834 by John Herschel. [5] [6]

Contents

Two supernovae have been observed in NGC 644: SN 2011gm (type Ia, mag. 15.8), [7] and SN 2018cmj (type II, mag. 17.1). [8]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 935 and IC 1801</span> Pair of interacting galaxies in the constellation Aries

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<span class="mw-page-title-main">NGC 5490</span> Radio galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 23</span> Galaxy in the constellation Pegasus

NGC 23 is a spiral galaxy located in the northern constellation of Pegasus, around 173.5 megalight-years distant from the Milky Way. It was discovered by William Herschel on 10 September 1784. In the Webb Society Deep-Sky Observer's Handbook, the visual appearance of NGC 23 is described as follows:

Bright, extended ellipse; a bright nuclear structure is noticeably elongated; two weak spiral enhancements emerge from opposite sides of the nucleus, one curving towards a bright star attached on the south end. The galaxy is likely interacting with NGC 9.

<span class="mw-page-title-main">NGC 4217</span> Spiral galaxy in constellation Canes Venatici

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<span class="mw-page-title-main">NGC 2748</span> Galaxy in the constellation Camelopardalis

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−3.6
×107 M
, or 44 million times the mass of the Sun.

<span class="mw-page-title-main">NGC 109</span> Spiral galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 2613</span> Spiral galaxy in the constellation Pyxis

NGC 2613 is a spiral galaxy in the southern constellation of Pyxis, next to the western constellation border with Puppis. It was discovered by the German-born astronomer William Herschel on November 20, 1784. With an apparent visual magnitude of 10.5, the galaxy is faintly visible using a telescope with a 100 mm (4 in) aperture. It appears spindle-shaped as it is almost edge-on to observers on Earth.

<span class="mw-page-title-main">NGC 1084</span> Galaxy in the constellation Eridanus

NGC 1084 is an unbarred spiral galaxy in the constellation Eridanus. It is located at a distance of about 63 million light-years away from the Milky Way. The galaxy was discovered by William Herschel on 10 January 1785. It has multiple spiral arms, which are not well defined. It belongs in the same galaxy group with NGC 988, NGC 991, NGC 1022, NGC 1035, NGC 1042, NGC 1047, NGC 1052 and NGC 1110. This group is in turn associated with the Messier 77 group.

<span class="mw-page-title-main">NGC 560</span> Galaxy in the constellation Cetus

NGC 560 is a lenticular galaxy in the constellation Cetus. It is estimated to be about 250 million light-years from the Milky Way and has a diameter of approximately 150,000 light years. It is part of the Abell 194 galaxy cluster. NGC 560 was discovered on October 1, 1785 by the German-British astronomer William Herschel.

<span class="mw-page-title-main">NGC 2227</span> 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 550</span> Spiral galaxy in the constellation Cetus

NGC 550 is a spiral galaxy in the constellation Cetus. It is estimated to be about 300 million light-years from the Milky Way and has a diameter of approximately 110,000 light years. The German-British astronomer William Herschel discovered it on 8 October 1785.

<span class="mw-page-title-main">NGC 812</span> Spiral galaxy in the constellation Andromeda

NGC 812 is a spiral galaxy located in the Andromeda constellation, an estimated 175 million light-years from the Milky Way. NGC 812 was discovered on December 11, 1876 by astronomer Édouard Stephan.

<span class="mw-page-title-main">NGC 813</span> Lenticular galaxy in the constrellation Hydrus

NGC 813 is a lenticular galaxy in the constellation Hydrus. It is estimated to be 390 million light-years from the Milky Way and has a diameter of approximately 140,000 ly. NGC 813 was discovered on November 24, 1834, by the British astronomer John Herschel.

<span class="mw-page-title-main">NGC 996</span> Galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 941</span> Spiral galaxy in the constellation Cetus

NGC 941 is an intermediate spiral galaxy in the constellation Cetus. It is an estimated 16.83 MPc from the Milky Way and has a diameter of approximately 55,000 light years. The galaxies NGC 926, NGC 934, NGC 936, NGC 955 are located in the same sky area. NGC 941 was discovered by the astronomer William Herschel on 6 January 1785.

<span class="mw-page-title-main">NGC 706</span> Galaxy in the constellation Pisces

NGC 706 is a spiral galaxy located in the Pisces constellation about 230 million light years from the Milky Way. It was discovered by the German–British astronomer William Herschel in 1786.

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 3 4 "NGC 644". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-05-20.
  3. Tully, R. Brent; Courtois, Hélène M.; Sorce, Jenny G. (2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 21. arXiv: 1605.01765 . Bibcode:2016AJ....152...50T. doi: 10.3847/0004-6256/152/2/50 . S2CID   250737862. 50.
  4. 1 2 3 "Results for object NGC 0644 (NGC 644)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-05-20.
  5. Ford, Dominic. "The galaxy NGC 644 - In-The-Sky.org". in-the-sky.org. Retrieved 2020-04-03.
  6. "Revised NGC Data for NGC 644". spider.seds.org. Retrieved 2020-04-03.
  7. Transient Name Server entry for SN 2011gm. Retrieved 24 March 2023.
  8. Transient Name Server entry for SN 2018cmj. Retrieved 24 March 2023.