NGC 3923

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NGC 3923
NGC 3923.png
NGC 3923 by imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Hydra
Right ascension 11h 51m 01.7118s [1]
Declination −28° 48′ 21.386″ [1]
Redshift 0.005801 +/- 0.00003 [1]
Heliocentric radial velocity 1739 ± 9 km/s [1]
Distance 71 ± 23 Mly (21.6 ± 7.0 Mpc) [1]
Apparent magnitude  (V)9.6
Characteristics
Type E4-5 [1]
Size~264,700  ly (81.16  kpc) (estimated) [1]
Apparent size  (V)5.9′ × 3.9′ [1]
Notable featuresShell galaxy
Other designations
ESO 440- G 017, AM 1148-283, MCG -05-28-012, PGC 37061 [1]

NGC 3923 is an elliptical galaxy located in the constellation Hydra. It is located at a distance of about 90 million light years from Earth, which, given its apparent dimensions, means that NGC 3923 is about 155,000 light years across. NGC 3923 is an example of a shell galaxy where the stars in its halo are arranged in layers. It has more than twenty shells. [2] It was discovered by William Herschel on March 7, 1791.

Contents

Characteristics

NGC 3923 imaged by the Cerro Tololo Inter-American Observatory NGC 3923 (noirlab2325d).jpg
NGC 3923 imaged by the Cerro Tololo Inter-American Observatory

NGC 3923 is an example of a shell galaxy where the stars in its halo are arranged in layers. NGC 3923 has up to 42 shells, the highest number among all shell galaxies, [3] and its shells are much more subtle than those of other shell galaxies. The shells of this galaxy are also symmetrical, while other shell galaxies are more skewed and asymmetrical. Concentric shells of stars enclosing a galaxy are quite common and are observed in many elliptical galaxies. In fact, every tenth elliptical galaxy exhibits this onion-like structure, which has never been observed in spiral galaxies. The shell-like structures are thought to develop as a consequence of galactic cannibalism, when a larger galaxy ingests a smaller companion. As the two centers approach, they initially oscillate about a common center, and this oscillation ripples outwards forming the shells of stars just as ripples on a pond spread when the surface is disturbed. [2]

Deep imaging also detected a stream extending from the core of NGC 3923 and a small elliptical galaxy on its axis, which is a probable progenitor of some of the shells. Another stream lies south of the core of NGC 3923, and a hook like structure lies at the northwest. [3]

Based on the velocity dispersion of the globular clusters of NGC 3923 the mass of the supermassive black hole of the galaxy was estimated to be (5.3±2.5)×108 M☉. [4]

Supernova

One supernova has been observed in NGC 3923. SN 2018aoz (type Ia, mag. 15.1) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 2 April 2018. [5] [6] It reached magnitude 12.7, making it tied with SN 2018pv for the brightest supernova of 2018. [7]

Nearby galaxies

NGC 3923 is the brightest galaxy in a galaxy group known as the NGC 3923 galaxy group. Within 25 arcminutes from NGC 3923 have been detected seven dwarf elliptical galaxies. NGC 3904 is located 37 arcminutes away. [8] Other galaxies in the group include NGC 3885, ESO 440-27, and ESO 440-011. Other nearby galaxies include NGC 3617, NGC 3673, NGC 3717, NGC 3936, and NGC 4105. [9]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 1395</span> Galaxy in the constellation Eridanus

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<span class="mw-page-title-main">NGC 1380</span> Galaxy in the constellation Fornax

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<span class="mw-page-title-main">NGC 4636</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 2525</span> Galaxy in the constellation Puppis

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<span class="mw-page-title-main">NGC 2832</span> Elliptical galaxy in the constellation Lynx

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References

  1. 1 2 3 4 5 6 7 8 9 "NASA/IPAC Extragalactic Database". Results for object NGC 3923. Retrieved 2016-01-18.
  2. 1 2 "Hubble Spots the Layers of NGC 3923". NASA. May 15, 2015.
  3. 1 2 Bílek, M.; Cuillandre, J.-C.; Gwyn, S.; Ebrová, I.; Bartošková, K.; Jungwiert, B.; Jílková, L. (22 March 2016). "Deep imaging of the shell elliptical galaxy NGC 3923 with MegaCam". Astronomy & Astrophysics. 588: A77. arXiv: 1505.07146 . Bibcode:2016A&A...588A..77B. doi:10.1051/0004-6361/201526608. S2CID   55565466.
  4. ↑ Sadoun, Raphael; Colin, Jacques (11 October 2012). "-σ relation between supermassive black holes and the velocity dispersion of globular cluster systems". Monthly Notices of the Royal Astronomical Society: Letters. 426 (1): L51–L55. arXiv: 1204.0144 . Bibcode:2012MNRAS.426L..51S. doi: 10.1111/j.1745-3933.2012.01321.x . S2CID   117185846.
  5. ↑ Sand, D.; Valenti, S.; Wyatt, S.; Bostroem, K. A.; Reichart, D. E.; Haislip, J. B.; Kouprianov, V. (2018). "Discovery and Spectroscopic Classification of DLT18q/AT2018aoz as a young type Ia Supernova". The Astronomer's Telegram. 11496: 1. Bibcode:2018ATel11496....1S.
  6. ↑ "SN 2018aoz". Transient Name Server. IAU . Retrieved 9 December 2024.
  7. ↑ Bishop, David. "Bright Supernovae - 20168". Rochester Astronomy. Retrieved 9 December 2024.
  8. ↑ Sandage, A., Bedke, J. (1994). The Carnegie Atlas of Galaxies. Carnegie Institution of Washington.{{cite book}}: CS1 maint: multiple names: authors list (link)
  9. ↑ Makarov, Dmitry; Karachentsev, Igor (21 April 2011). "Galaxy groups and clouds in the local (z~ 0.01) Universe". Monthly Notices of the Royal Astronomical Society. 412 (4): 2498–2520. arXiv: 1011.6277 . Bibcode:2011MNRAS.412.2498M. doi: 10.1111/j.1365-2966.2010.18071.x . S2CID   119194025.
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